3 The catalogue

The main catalogue is presented in Table 1. This table includes collated data for all the symbiotic stars we know of. Note that a colon indicates an uncertain measurement or an estimate. Stars are ordered by right ascension (RA) for the equinox J2000.0. The content of each column is described below.

1: Symbiotic star catalogue number. A star symbol, if present here, means that there is a classification note and/or comment for the given object. We would still advise the use of the symbiotic (or suspected symbiotic) star name, as given in the second column of Tables 1 and 2, and not the object's catalogue number.

2: Symbiotic star name. If, for a given object, a variable star name exists, then it was chosen; otherwise, the name used most often in the literature was adopted.

3,4: RA and declination (J2000.0), taken from radio VLA positions (Ivison et al. 1995,Seaquist & Taylor 1990,Seaquist et al. 1984) if available, and if not from the SIMBAD database but corrected in a few cases were obvious mistakes have been spotted. If position was taken from somewhere else then comment is given in Sect. 4.

5,6: Galactic coordinates (not included for extragalactic objects).

7,8: Magnitudes in the V and K filters, respectively. As most (if not all) symbiotics are variable, these values are arbitrary (usually the average of published measurements) just to give the general level of an object's brightness.

9: IR type. If two IR types are given for one object, we supply references to both estimates in the notes.

10: Information on whether an IUE spectrum (or spectra) is (are) available (+) or not (-). The number of spectra can be readily obtained from SIMBAD (http://simbad.u-strasbg.fr/Simbad) and the spectra can be obtained from the IUE data archives (http://nssdca.gsfc.nasa.gov/ndads).

11: Information about whether an object was ever detected in X-rays. Plus (+) means a detection; minus (-) means that an object was observed but not detected and that only an upper limit is available. Most of the detections and upper limits came from ROSAT and were reported in Bickert et al. 1997 but some have also been observed by Einstein Allen 1981, EXOSAT and ASCA.

12: Highest ionization potential ever observed in the emission-line spectra of an object. The potential is given in electron volts (eV).

13: The symbiotic star catalogue number (repeated).

14: An estimate of the spectral type of the cool component, with references. Since the blue and visual spectral regions are often contaminated by the circumstellar nebula and/or the hot component, we have given priority to estimates made in the near-IR region and, in the case of multiple estimates, to those made at quiescence and/or near to inferior conjunction of the cool giant. The estimates based on the TiO bands are separated from those based on CO 2.3- $\mu$ m bands by "/''. Also, if the cool component was reported to behave as a Mira (i.e. if Mira-like pulsations have been detected or the object's position in the near-IR/IRAS colour diagram coincides with the region occupied by Mira variables Kenyon & Fernandez-Castro 1987,Whitelock 1988) then it is noted in this column.

15: Radio observations of symbiotics. Detections or upper limits are given. In parentheses, the wavelength of observation is reported. If more than one detection has been reported, only one is included and the priority is given to the most extensive radio survey of symbiotics at 3.6 cm Seaquist et al. 1993. Other extensive surveys of symbiotic stars which were searched for radio detection include Seaquist & Taylor 1990,Wright & Allen 1978,Seaquist et al. 1984,Ivison et al. 1991,Ivison et al. 1995.

16,17: IRAS fluxes at 12 and 25 $\mu$ m. The fluxes are taken from pointed observations, if available, Kenyon et al. 1988 or from survey observations as listed in SIMBAD. If, for some object, there was no report of observations in either of the above two sources, but IRAS fluxes were available from somewhere else, then the reference to reported observations is given in the notes. The upper limits are marked with capital L. The IRAS number is listed in Table 8 (which contains different object names for the symbiotic and suspected symbiotic stars). If the number is not there then the reference to the reported observations is given in the section containing comments.

18: Major literature references to the object. A number indicates the reference number; abbreviations in parentheses mark the subject the reference was noted for: fc - finding chart, spc - optical spectrum, class - classification, parm - the latest or the most extensive and up-to-date discussion of an object.

In Table 2, we present data for objects suspected of being symbiotic stars. The order and content of the columns is exactly the same as in Table 1. The catalogue numbers of suspected symbiotic stars are preceded by the letter "s'' throughout the catalogue.

The next two tables include data on symbiotic and suspected symbiotic star orbits. In Table 3, we have put orbital photometric ephemerides, including information on the presence of eclipses if available, and references to every ephemeris estimate. In Table 4, the reader will find the orbital elements of twenty symbiotic stars as well as spectroscopic periods, radial velocity semi-amplitudes for the cool components, mass ratios, systemic velocities, eccentricities, times of inferior spectroscopic conjunctions of the giant, sizes of the giant orbits, mass functions and references to each orbital estimate.

In Table 5, we have collected the pulsation ephemerides for Miras in symbiotic and suspected symbiotic stars. Again, a reference to every estimate is given.

Table 6 includes known Hipparcos parallaxes for symbiotic stars, however for most objects uncertainities are very high and parallax estimations may not be significant.

Table 7 includes information on symbiotic and suspected symbiotic star flickering and outburst characteristics.

Table 8 includes most of different names for symbiotic and suspected symbiotic stars. Symbiotic stars appear first, then suspected symbiotic stars follow. Objects are first listed by their catalogue number, then by the name (translated to SIMBAD nomenclature, if possible -- the name by which the object is known in Tables 1 or 2), then other names are given. The names are compatible with SIMBAD and general internet database nomenclature. In some cases, the catalogue name differs between Table 1 (or 2) and Table 8. This discrepancy is due the most commonly accepted name (Tables 1 or 2) not following SIMBAD nomenclature (Table 8).

Table 1: Symbiotic star
No. Name $\alpha$ (2000) $\delta$ (2000) $l^{\rm II}$ $b^{\rm II}$ V K IR IUE X IP $_{\rm max}$

$^{\rm h}$ $^{\rm m}$ $^{\rm s}$ $^\circ$ ' '' $^\circ$ $^\circ$ [mag] [mag] [eV]

001 SMC1 00 29 10.9 -74 57 38.9 16.2 S: + 114

002 SMC2 00 42 48.1 -74 42 00.0 16.2 S: + - 114

003 EG And 00 44 37.1 +40 40 45.7 121.54 -22.17 7.1 2.6 S + + 100

004 $^\star$ SMC3 00 48 19.9 -73 31 54.9 15.5: S: + + 235

005 $^\star$ SMC N60 00 57 12.0 -74 13 00.0 16.8 13.0 S,D + - 114

006 LIN 358 00 59 24.0 -75 04 59.9 15.2 11.4 S + + 114

007 SMC N73 01 04 42.0 -75 48 00.0 15.5 11.6 S + - 114

008 $^\star$ AX Per 01 36 22.7 +54 15 02.5 129.53 -8.04 10.9 5.5 S + - 109.3

009 $^\star$ V471 Per 01 58 49.6 +52 53 48.9 133.12 -8.64 13.0 9.8 D' + - 77.5

010 $^\star$ o Ceti 02 19 20.7 -02 58 39.5 167.76 -57.98 6.0 -2.7 + + 54.4

011 $^\star$ BD Cam 03 42 09.3 +63 13 00.5 140.84 +6.44 5.1 0.2 + 77.5

012 S32 04 37 45.0 -01 19 05.9 197.48 -30.04 13.5 S + + 114

013 LMC S154 04 51 50.2 -75 03 36.0 15.7 10.1 D + - 114

014 LMC S147 04 54 04.6 -70 59 34.0 16.0 11.9 S + 114

015 LMC N19 05 03 24.0 -67 56 35.0 16.4 - 114

016 $^\star$ UV Aur 05 21 48.8 +32 30 43.1 174.22 -2.35 8.5 2.1 S + - 41.0

017 $^\star$ V1261 Ori 05 22 18.6 -08 39 58.0 210.63 -23.72 6.8 2.1 + + 77.5

018 $^\star$ LMC1 05 25 01.0 -62 28 46.9 15.9 9.9 D + 97.1

019 LMC N67 05 36 02.8 -64 43 23.9 15.9 11.4 S + - 77.5

020 $^\star$ Sanduleak's star 05 45 19.6 -71 16 09.9 16.9 13.0 D: + - 114

021 LMC S63 05 48 44.1 -67 36 12.9 15.2 11.3 S + + 97.1

022 SMP LMC 94 05 54 10.3 -73 02 39.0 + 114

023 $^\star$ BX Mon 07 25 24.0 -03 36 00.0 220.04 +5.88 11.7 5.7 S + - 54.4

024 $^\star$ V694 Mon 07 25 51.2 -07 44 08.0 223.76 +4.05 9.5 5.1 S + - 24.6

025 WRAY 15-157 08 06 34.8 -28 31 57.0 246.60 +1.95 13.2 9.4 D' - 54.4

026 $^\star$ RX Pup 08 14 12.3 -41 42 29.0 258.50 -3.93 11.5 2.8 D + + 114

027 $^\star$ Hen 3-160 08 24 52.8 -51 28 36.0 267.68 -7.87 15.4 7.5 S - 114

028 $^\star$ AS 201 08 31 42.9 -27 45 32.0 249.08 +6.97 11.8 9.9 D' + - 54.4

029 $^\star$ KM Vel 09 41 14.0 -49 22 47.0 274.19 +2.58 15.0 5.7 D - 41.0

030 V366 Car 09 54 43.3 -57 18 52.4 280.81 -2.24 13.0 4.7 D + - 114

031 Hen 3-461 10 39 08.5 -51 24 11.9 282.90 +6.25 12.3 3.9 S - 100

032 $^\star$ SS73 29 11 08 27.4 -65 47 17.9 292.63 -5.00 14.1 10.6 S + - 100

033 $^\star$ SY Mus 11 32 05.5 -65 25 08.0 294.80 -3.81 10.9 4.7 S + - 114

034 $^\star$ BI Cru 12 23 26.0 -62 38 16.0 299.72 +0.06 11.1 5.0 D + - 75.5

035 RT Cru 12 34 54.0 -64 33 54.0 301.16 -1.75 12.6 54.4

036 $^\star$ TX CVn 12 44 42.0 +36 45 50.6 130.93 +80.26 9.5 6.3 S + - 13.6

037 Hen 2-87 12 45 20.1 -63 00 39.9 302.24 -0.15 15.5 6.0 S - 114

038 $^\star$ Hen 3-828 12 50 58.0 -57 50 47.0 302.87 +5.03 13.4 7.1 S - 100

039 SS73 38 12 51 26.2 -64 59 58.1 302.93 -2.13 14.5 6.1 D 108.8

040 Hen 3-863 13 07 43.8 -48 00 23.0 305.75 +14.78 11.8 8.5 S - 54.4

041 $^\star$ St 2-22 13 14 30.0 -58 51 47.9 305.92 +3.87 8.5 S - 114

042 CD-36 8436 13 16 01.6 -37 00 11.9 308.37 +25.61 11.2 5.7 S - 54.4

043 $^\star$ V840 Cen 13 20 46.9 -55 50 35.9 307.07 +6.79 14.1 10.8 54.4

044 Hen 3-905 13 30 37.2 -57 58 18.0 308.12 +4.50 13.4 8.5 S 114

045 RW Hya 13 34 17.8 -25 22 52.1 314.99 +36.49 8.9 4.7 S + - 77.5

046 $^\star$ Hen 3-916 13 35 28.9 -64 45 45.0 307.61 -2.29 12.9 7.8 S - 114

047 $^\star$ V704 Cen 13 54 56.2 -58 27 16.9 311.17 +3.40 13.5 8.4 D - 54.4

048 $^\star$ V852 Cen 14 11 52.1 -51 26 23.8 315.48 +9.46 14.0 6.9 D + - 100

049 V835 Cen 14 14 09.4 -63 25 46.1 312.03 -2.03 12.9 5.0 D + - 114

050 $^\star$ V417 Cen 14 15 55.9 -61 53 53.9 312.71 -0.64 12.2 D' 35.1

**Table 1:** Symbiotic star
No.	Name	$\alpha$ (2000)	$\delta$ (2000)	$l^{\rm II}$	$b^{\rm II}$	V	K	IR	IUE	X	IP $_{\rm max}$
		$^{\rm h}$ $^{\rm m}$ $^{\rm s}$	$^\circ$ ' ''	$^\circ$	$^\circ$	[mag]	[mag]				[eV]
001	SMC1	00 29 10.9	-74 57 38.9			16.2		S:	+		114
002	SMC2	00 42 48.1	-74 42 00.0			16.2		S:	+	-	114
003	EG And	00 44 37.1	+40 40 45.7	121.54	-22.17	7.1	2.6	S	+	+	100
004 $^\star$	SMC3	00 48 19.9	-73 31 54.9			15.5:		S:	+	+	235
005 $^\star$	SMC N60	00 57 12.0	-74 13 00.0			16.8	13.0	S,D	+	-	114
006	LIN 358	00 59 24.0	-75 04 59.9			15.2	11.4	S	+	+	114
007	SMC N73	01 04 42.0	-75 48 00.0			15.5	11.6	S	+	-	114
008 $^\star$	AX Per	01 36 22.7	+54 15 02.5	129.53	-8.04	10.9	5.5	S	+	-	109.3
009 $^\star$	V471 Per	01 58 49.6	+52 53 48.9	133.12	-8.64	13.0	9.8	D'	+	-	77.5
010 $^\star$	o Ceti	02 19 20.7	-02 58 39.5	167.76	-57.98	6.0	-2.7		+	+	54.4
011 $^\star$	BD Cam	03 42 09.3	+63 13 00.5	140.84	+6.44	5.1	0.2		+		77.5
012	S32	04 37 45.0	-01 19 05.9	197.48	-30.04	13.5		S	+	+	114
013	LMC S154	04 51 50.2	-75 03 36.0			15.7	10.1	D	+	-	114
014	LMC S147	04 54 04.6	-70 59 34.0			16.0	11.9	S	+		114
015	LMC N19	05 03 24.0	-67 56 35.0			16.4				-	114
016 $^\star$	UV Aur	05 21 48.8	+32 30 43.1	174.22	-2.35	8.5	2.1	S	+	-	41.0
017 $^\star$	V1261 Ori	05 22 18.6	-08 39 58.0	210.63	-23.72	6.8	2.1		+	+	77.5
018 $^\star$	LMC1	05 25 01.0	-62 28 46.9			15.9	9.9	D	+		97.1
019	LMC N67	05 36 02.8	-64 43 23.9			15.9	11.4	S	+	-	77.5
020 $^\star$	Sanduleak's star	05 45 19.6	-71 16 09.9			16.9	13.0	D:	+	-	114
021	LMC S63	05 48 44.1	-67 36 12.9			15.2	11.3	S	+	+	97.1
022	SMP LMC 94	05 54 10.3	-73 02 39.0						+		114
023 $^\star$	BX Mon	07 25 24.0	-03 36 00.0	220.04	+5.88	11.7	5.7	S	+	-	54.4
024 $^\star$	V694 Mon	07 25 51.2	-07 44 08.0	223.76	+4.05	9.5	5.1	S	+	-	24.6
025	WRAY 15-157	08 06 34.8	-28 31 57.0	246.60	+1.95	13.2	9.4	D'		-	54.4
026 $^\star$	RX Pup	08 14 12.3	-41 42 29.0	258.50	-3.93	11.5	2.8	D	+	+	114
027 $^\star$	Hen 3-160	08 24 52.8	-51 28 36.0	267.68	-7.87	15.4	7.5	S		-	114
028 $^\star$	AS 201	08 31 42.9	-27 45 32.0	249.08	+6.97	11.8	9.9	D'	+	-	54.4
029 $^\star$	KM Vel	09 41 14.0	-49 22 47.0	274.19	+2.58	15.0	5.7	D		-	41.0
030	V366 Car	09 54 43.3	-57 18 52.4	280.81	-2.24	13.0	4.7	D	+	-	114
031	Hen 3-461	10 39 08.5	-51 24 11.9	282.90	+6.25	12.3	3.9	S		-	100
032 $^\star$	SS73 29	11 08 27.4	-65 47 17.9	292.63	-5.00	14.1	10.6	S	+	-	100
033 $^\star$	SY Mus	11 32 05.5	-65 25 08.0	294.80	-3.81	10.9	4.7	S	+	-	114
034 $^\star$	BI Cru	12 23 26.0	-62 38 16.0	299.72	+0.06	11.1	5.0	D	+	-	75.5
035	RT Cru	12 34 54.0	-64 33 54.0	301.16	-1.75	12.6					54.4
036 $^\star$	TX CVn	12 44 42.0	+36 45 50.6	130.93	+80.26	9.5	6.3	S	+	-	13.6
037	Hen 2-87	12 45 20.1	-63 00 39.9	302.24	-0.15	15.5	6.0	S		-	114
038 $^\star$	Hen 3-828	12 50 58.0	-57 50 47.0	302.87	+5.03	13.4	7.1	S		-	100
039	SS73 38	12 51 26.2	-64 59 58.1	302.93	-2.13	14.5	6.1	D			108.8
040	Hen 3-863	13 07 43.8	-48 00 23.0	305.75	+14.78	11.8	8.5	S		-	54.4
041 $^\star$	St 2-22	13 14 30.0	-58 51 47.9	305.92	+3.87		8.5	S		-	114
042	CD-36 8436	13 16 01.6	-37 00 11.9	308.37	+25.61	11.2	5.7	S		-	54.4
043 $^\star$	V840 Cen	13 20 46.9	-55 50 35.9	307.07	+6.79	14.1	10.8				54.4
044	Hen 3-905	13 30 37.2	-57 58 18.0	308.12	+4.50	13.4	8.5	S			114
045	RW Hya	13 34 17.8	-25 22 52.1	314.99	+36.49	8.9	4.7	S	+	-	77.5
046 $^\star$	Hen 3-916	13 35 28.9	-64 45 45.0	307.61	-2.29	12.9	7.8	S		-	114
047 $^\star$	V704 Cen	13 54 56.2	-58 27 16.9	311.17	+3.40	13.5	8.4	D		-	54.4
048 $^\star$	V852 Cen	14 11 52.1	-51 26 23.8	315.48	+9.46	14.0	6.9	D	+	-	100
049	V835 Cen	14 14 09.4	-63 25 46.1	312.03	-2.03	12.9	5.0	D	+	-	114
050 $^\star$	V417 Cen	14 15 55.9	-61 53 53.9	312.71	-0.64	12.2		D'			35.1

**Table 1:** continued
No.	Cool-star spectrum	Radio	IRAS	IRAS	References
		[mJy]	F₁₂[Jy]	F₂₅[Jy]
001	C3.2:,C(Mürset et al. 1996,Morgan 1992)				Morgan 1992 (fc,spc,class) Mürset et al. 1996 (parm)
002	K,G-K(Mürset et al. 1996,Morgan 1992)				Morgan 1992 (fc,spc,class) Mürset et al. 1996 (parm)
003	M3(Mürset & Schmid 1999)	0.54(3.6 cm)	4.5	1.25	Allen 1984 (fc,class) Kenyon 1986 (spc) Wilson & Vaccaro 1997 (parm)
004	M0,K-M(Morgan 1992,Mürset et al. 1996)				Morgan 1992 (fc,spc,class) Jordan et al. 1996 (parm)
005	C3.3(Mürset et al. 1996)				Allen 1984 (fc,class) Mürset et al. 1996 (spc,parm)
006	mid K(Mürset et al. 1996)				Allen 1984 (fc,class) Mürset et al. 1996 (spc,parm)
007	K7(Mürset et al. 1996)				Allen 1984 (fc,class) Mürset et al. 1996 (spc,parm)
008	M6(Mürset & Schmid 1999)	0.58(3.6 cm)	0.32	0.10	Allen 1984 (fc,class) Miko $\l$ ajewska & Kenyon 1992,Ivison et al. 1993 (spc,parm)
009	G5(Mürset & Schmid 1999)	0.45(3.6 cm)	1.6	2.7	Allen 1984 (fc,class) Blair et al. 1983 (spc,parm)
010	Mira,M2-7(Whitelock 1988,Karovska et al. 1997)		4881	2261	Yamashita & Maehara 1977 (spc) Karovska et al. 1997 (parm) Belczynski 2000 (class)
011	M3,S5.3(Adelman 1998,Keenan 1954)	0.18(3.6 cm)	40.95	10.82	Keenan 1954 (spc) Adelman 1998 (parm) Belczynski 2000 (class)
012	C1.1CH(Schmid 1994)				Henden & Munari2000 (fc) Downes & Keyes 1988 (class) Schmid 1994 (spc) Schmid & Nussbaumer 1993 (parm)
013	C2.2(Mürset et al. 1996)				Remillard et al. 1992 (fc) Mürset et al. 1996 (class,spc,parm)
014	M1,K5(Mürset et al. 1996,Morgan & Allen1988)				Morgan & Allen1988 (fc,spc,class) Mürset et al. 1996 (parm)
015	M4(Morgan 1996)				Bohannan 1974 (fc) Morgan 1996 (class,spc,parm)
016	Mira C8.1Je(Olson & Richer 1975)	<0.34(3.6 cm)	65	21	Allen 1984 (fc,spc,class) Reimers & Groote 1983 (parm)
017	S4.1,M3(Jorissen et al. 1996,Ake et al. 1991)	<0.1(3.6 cm)	7.98	2.01	Belczynski 2000 (class) Jorissen et al. 1996 (parm)
018	C4.3,C(Mürset et al. 1996,Morgan 1992)				Morgan 1992 (fc,spc,class) Mürset et al. 1996 (parm)
019	C3.2,C(Mürset et al. 1996,Cowley et al. 1989)				Henize 1956 (fc) Cowley et al. 1989 (spc,class) Mürset et al. 1996 (parm)
020					Allen 1984 (fc) Belczynski 2000 (class) Mürset et al. 1996 (spc,parm)
021	C2.1J(Mürset et al. 1996)				Allen 1984 (fc,class) Mürset et al. 1996 (spc,parm)
022	M(Kontizas et al. 1996)				Leisy et al. 1997 (fc) Meatheringham & Dopita 1991 (spc,class)
023	M5(Mürset & Schmid 1999)	<0.07(3.6 cm)	0.32	0.09L	Allen 1984 (fc,class,spc) Dumm et al. 1998 (parm)
024	M6(Mürset & Schmid 1999)		0.84	0.36:	Belczynski 2000 (class) Panferov et al. 1997 (spc,parm)
025	G5(Mürset & Schmid 1999)	0.34(3.6 cm)	1.0	1.3	Allen 1984 (fc,class,spc)
026	Mira M5.5/M5(Mürset & Schmid 1999,Allen 1980)	12.6 $\div$ 69.7(3.6 cm)	220	132	Allen 1984 (fc,class) Miko $\l$ ajewska et al. 1999 (spc,parm)
027	M7(Mürset & Schmid 1999,Allen 1980)	<17(6 cm)	0.12	0.03L	Allen 1984 (fc,class,spc)
028	G5(Mürset & Schmid 1999)	0.69(3.6 cm)	1.1	2.8	Allen 1984 (fc,class,spc) Schwarz 1991 (parm)
029	Mira,M(Whitelock 1988,Acker et al. 1988)	1.49(3.5 cm)	11.84	7.81	Dopita & Hua 1997,Viotti et al. 1986 (spc) Belczynski 2000 (class) Feast et al. 1983 (parm)
030	Mira M6(Mürset & Schmid 1999)	1.73(3.5 cm)	9.5	4.3	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
031	M6(Mürset & Schmid 1999)		2.02	0.61	Allen 1984 (fc) Pereira et al. 1998 (spc,class)
032	G/K(Allen 1982,Munari & Buson 1994)	<16(6 cm)	0.07	0.11L	Allen 1984 (fc,class,spc) Munari & Buson 1994 (parm)
033	M5(Mürset & Schmid 1999)	<12(6 cm)	1.00	0.40	Allen 1984 (fc,class,spc) Schmutz et al. 1994 (parm)
034	Mira M0-1(Schulte-Ladbeck 1988)	5.11(3.5 cm)	18.3	15.5	Allen 1984 (fc,class,spc) Rossi et al. 1988 (spc) Harries 1996 (parm)
035	M4-5(Cieslinski et al. 1994)				Cieslinski et al. 1994 (spc,class,parm)
036	early M,K5.3(Kenyon 1986,Kenyon & Fernandez-Castro 1987)	<0.06(3.6 cm)	1.10	0.38	Kenyon 1986 (spc,class) Kenyon & Garcia 1989 (parm)
037	M5.5/M7.5(Mürset & Schmid 1999,Allen 1980)	<12(6 cm)	0.40	1.2L	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
038	M6(Mürset & Schmid 1999,Allen 1980)	<16(6 cm)	0.11	0.06	Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc,parm)
039	Mira C9(Schulte-Ladbeck et al. 1988)	5.12(3.5 cm)	7.4	3.1	Allen 1984 (fc,class,spc)
040	K4:(Allen 1980)	<12(6 cm)			Allen 1984 (fc,class,spc)
041	M4.5(Mürset & Schmid 1999)				Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
042	M5.5(Mürset & Schmid 1999)	<0.24(6 cm)	0.40	0.25L	Allen 1984 (fc) Gutierrez-Moreno et al. 1992 (spc,class,parm)
043	K5(Duerbeck & Seitter 1989)		0.03L	0.22L	McNaught & Dawes 1986 (fc) Duerbeck & Seitter 1989 (spc,class,parm)
044	M3(Mürset & Schmid 1999)	<13(6 cm)			Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc,parm)
045	M2(Mürset & Schmid 1999)	0.60(3.6 cm)	0.83	0.36	Allen 1984 (fc,class,spc) Schild et al. 1996 (parm)
046	M5/M6(Mürset & Schmid 1999,Allen 1980)	<20(6 cm)			Allen 1984,Harries & Howarth 1996 (fc) Allen 1984 (class,spc)
047	M6.5(Mürset & Schmid 1999)		1.43	1.16	Allen 1984 (fc) Pereira et al. 1998 (spc) Gutierrez-Moreno et al. 1992 (class,parm)
048	Mira(Whitelock 1988)	3.31(3.5 cm)	8.8	9.2	Allen 1984 (fc,spc) Belczynski 2000 (class) de Freitas Pacheco & Costa 1996 (parm)
049	Mira $\geq$ M5(Schulte-Ladbeck 1988)	5.79(3.5 cm)	32.6	24.3	Allen 1984 (fc,class,spc) Gutierrez-Moreno & Moreno 1986 (parm)
050	G8-K2,G2(Cieslinski et al. 1998,van Winckel et al. 1994)		12.61	10.60	Cieslinski et al. 1994 (spc,class) van Winckel et al. 1994 (parm)

Table 1: continued
No. Name $\alpha$ (2000) $\delta$ (2000) $l^{\rm II}$ $b^{\rm II}$ V K IR IUE X IP $_{\rm max}$

$^{\rm h}$ $^{\rm m}$ $^{\rm s}$ $^\circ$ ' '' $^\circ$ $^\circ$ [mag] [mag] [eV]

051 BD-21 3873 14 16 34.3 -21 45 50.2 327.88 +36.95 10.7 7.2 S + - 77.5

052 Hen 2-127 15 24 49.8 -51 49 52.6 325.53 +4.19 16.0 8.1 D - 114

053 Hen 3-1092 15 47 10.6 -66 29 16.0 319.22 -9.35 13.5 7.8 S + - 114

054 Hen 3-1103 15 48 28.5 -44 19 00.9 333.21 +7.90 13.0 8.4 S - 114

055 $^\star$ HD 330036 15 51 15.9 -48 44 58.5 330.78 +4.15 11.0 7.6 D' + - 77.5

056 $^\star$ Hen 2-139 15 54 45.4 -55 29 36.9 326.91 -1.40 16.8 5.9 D - 35.1

057 T CrB 15 59 30.1 +25 55 12.6 42.37 +48.16 10.1 4.8 S + + 77.5

058 $^\star$ AG Dra 16 01 40.5 +66 48 09.5 100.29 +40.97 9.1 6.2 S + + 114

059 WRAY 16-202 16 06 56.8 -49 26 39.0 332.28 +1.96 6.8 S - 114

060 $^\star$ V347 Nor 16 14 00.3 -56 59 26.0 327.92 -4.30 16.6 5.0 D + - 54.4

061 UKS Ce-1 16 15 29.2 -22 12 15.9 353.02 +20.25 15.0 11.3 S - 54.4

062 QS Nor 16 21 07.9 -42 23 53.9 338.94 +5.36 13.3 8.1 S - 35.1

063 WRAY 15-1470 16 23 21.6 -27 40 13.0 350.06 +15.24 12.9 7.8 S - 54.4

064 Hen 2-171 16 34 03.9 -35 05 32.8 346.03 +8.55 14.8 6.7 D + - 235

065 $^\star$ Hen 3-1213 16 35 15.3 -51 42 24.0 333.87 -2.81 10.4 6.7 S + - 97.1

066 $^\star$ Hen 2-173 16 36 24.1 -39 51 52.4 342.77 +5.01 13.8 6.8 S - 54.4

067 $^\star$ Hen 2-176 16 41 31.2 -45 13 04.7 339.39 +0.74 15 5.7 S,D - 114

068 $^\star$ KX TrA 16 44 35.2 -62 37 14.0 326.41 -10.94 12.4 6.0 S + - 114

069 AS 210 16 51 20.4 -26 00 27.1 355.51 +11.55 12.2 6.5 D + - 114

070 HK Sco 16 54 39.0 -30 23 30.0 352.48 +8.27 13.5 7.9 S + - 114

071 $^\star$ CL Sco 16 54 51.9 -30 37 18.0 352.32 +8.09 13.3 7.9 S + - 54.9

072 MaC 1-3 17 01 27.9 -47 45 33.9 339.62 -3.52 18.2 D - 114

073 $^\star$ V455 Sco 17 07 21.5 -34 05 21.0 351.17 +3.90 13.7 5.9 S - 114

074 $^\star$ Hen 3-1341 17 08 36.6 -17 26 30.0 5.02 +13.39 12.5 7.6 S + - 114

075 Hen 3-1342 17 08 55.0 -23 23 35.0 0.08 +9.92 12.7 8.5 S - 114

076 AS 221 17 12 02.2 -32 34 24.9 352.98 +4.00 12.0 7.6 S - 114

077 $^\star$ H 2-5 17 15 19.0 -31 34 05.9 354.20 +4.02 5.5 S,D - 114

078 Sa 3-43 17 17 55.9 -30 01 48.0 355.79 +4.45 7.9 S - 54.4

079 Draco C-1 17 19 57.6 +57 50 04.9 17.0 11.4 + + 77.5

080 Th 3-7 17 21 02.4 -29 22 59.4 356.70 +4.27 14.0 8.1 S - 114

081 Th 3-17 17 27 31.9 -29 02 53.0 357.78 +3.27 14.0 8.2 S - 54.4

082 Th 3-18 17 28 27.0 -28 38 34.0 358.23 +3.33 12.6 8.2 S - 114

083 Hen 3-1410 17 29 06.0 -29 43 24.1 357.41 +2.61 12.8 8.5 S - 114

084 $^\star$ V2116 Oph 17 32 03.0 -24 44 44.3 1.94 +4.79 19.0 8.1 S + 235

085 Th 3-29 17 32 28.0 -29 05 06.0 358.34 +2.35 17.0 7.0 S - 35.1

086 Th 3-30 17 33 43.0 -28 07 18.0 359.30 +2.65 13.1 8.3 S - 114

087 Th 3-31 17 34 26.5 -29 28 05.0 358.25 +1.78 13.6 7.6 S - 114

088 $^\star$ M 1-21 17 34 17.2 -19 09 21.9 6.96 +7.36 13.7 7.2 S - 114

089 $^\star$ Hen 2-251 17 35 22.3 -29 45 20.0 358.12 +1.46 15.4 7.3 D - 114

090 Pt 1 17 38 49.8 -23 54 02.9 3.48 +3.94 15.0 8.6 S - 114

091 K 6-6 17 39 18.3 -28 15 06.9 359.85 +1.54 16.5 S - 114

092 $^\star$ RT Ser 17 39 51.8 -11 56 44.7 13.89 +9.97 15.0 7.0 S + - 114

093 $^\star$ AE Ara 17 41 04.9 -47 03 20.9 344.00 -8.66 12.5 6.4 S + - 77.5

094 $^\star$ SS73 96 17 41 28.3 -36 47 51.9 352.85 -3.38 15.2 6.4 S - 100

095 UU Ser 17 42 37.9 -15 24 29.9 11.23 +7.62 15.3 9.1 S - 114

096 $^\star$ V2110 Oph 17 43 33.3 -22 45 37.0 5.03 +3.62 19 7.9 D - 114

097 V916 Sco 17 43 54.9 -36 03 24.9 353.73 -3.41 8.3 S - 54.4

098 Hen 2-275 17 45 31.0 -38 39 47.9 351.67 -5.03 15.5 >9.3 S - 114

099 V917 Sco 17 48 04.0 -36 08 17.9 354.10 -4.17 13.0 7.9 S - 114

100 $^\star$ H 1-36 17 49 48.1 -37 01 27.9 353.51 -4.92 12.0 7.5 D + + 114

**Table 1:** continued
No.	Name	$\alpha$ (2000)	$\delta$ (2000)	$l^{\rm II}$	$b^{\rm II}$	V	K	IR	IUE	X	IP $_{\rm max}$
		$^{\rm h}$ $^{\rm m}$ $^{\rm s}$	$^\circ$ ' ''	$^\circ$	$^\circ$	[mag]	[mag]				[eV]
051	BD-21 3873	14 16 34.3	-21 45 50.2	327.88	+36.95	10.7	7.2	S	+	-	77.5
052	Hen 2-127	15 24 49.8	-51 49 52.6	325.53	+4.19	16.0	8.1	D		-	114
053	Hen 3-1092	15 47 10.6	-66 29 16.0	319.22	-9.35	13.5	7.8	S	+	-	114
054	Hen 3-1103	15 48 28.5	-44 19 00.9	333.21	+7.90	13.0	8.4	S		-	114
055 $^\star$	HD 330036	15 51 15.9	-48 44 58.5	330.78	+4.15	11.0	7.6	D'	+	-	77.5
056 $^\star$	Hen 2-139	15 54 45.4	-55 29 36.9	326.91	-1.40	16.8	5.9	D		-	35.1
057	T CrB	15 59 30.1	+25 55 12.6	42.37	+48.16	10.1	4.8	S	+	+	77.5
058 $^\star$	AG Dra	16 01 40.5	+66 48 09.5	100.29	+40.97	9.1	6.2	S	+	+	114
059	WRAY 16-202	16 06 56.8	-49 26 39.0	332.28	+1.96		6.8	S		-	114
060 $^\star$	V347 Nor	16 14 00.3	-56 59 26.0	327.92	-4.30	16.6	5.0	D	+	-	54.4
061	UKS Ce-1	16 15 29.2	-22 12 15.9	353.02	+20.25	15.0	11.3	S		-	54.4
062	QS Nor	16 21 07.9	-42 23 53.9	338.94	+5.36	13.3	8.1	S		-	35.1
063	WRAY 15-1470	16 23 21.6	-27 40 13.0	350.06	+15.24	12.9	7.8	S		-	54.4
064	Hen 2-171	16 34 03.9	-35 05 32.8	346.03	+8.55	14.8	6.7	D	+	-	235
065 $^\star$	Hen 3-1213	16 35 15.3	-51 42 24.0	333.87	-2.81	10.4	6.7	S	+	-	97.1
066 $^\star$	Hen 2-173	16 36 24.1	-39 51 52.4	342.77	+5.01	13.8	6.8	S		-	54.4
067 $^\star$	Hen 2-176	16 41 31.2	-45 13 04.7	339.39	+0.74	15	5.7	S,D		-	114
068 $^\star$	KX TrA	16 44 35.2	-62 37 14.0	326.41	-10.94	12.4	6.0	S	+	-	114
069	AS 210	16 51 20.4	-26 00 27.1	355.51	+11.55	12.2	6.5	D	+	-	114
070	HK Sco	16 54 39.0	-30 23 30.0	352.48	+8.27	13.5	7.9	S	+	-	114
071 $^\star$	CL Sco	16 54 51.9	-30 37 18.0	352.32	+8.09	13.3	7.9	S	+	-	54.9
072	MaC 1-3	17 01 27.9	-47 45 33.9	339.62	-3.52	18.2		D		-	114
073 $^\star$	V455 Sco	17 07 21.5	-34 05 21.0	351.17	+3.90	13.7	5.9	S		-	114
074 $^\star$	Hen 3-1341	17 08 36.6	-17 26 30.0	5.02	+13.39	12.5	7.6	S	+	-	114
075	Hen 3-1342	17 08 55.0	-23 23 35.0	0.08	+9.92	12.7	8.5	S		-	114
076	AS 221	17 12 02.2	-32 34 24.9	352.98	+4.00	12.0	7.6	S		-	114
077 $^\star$	H 2-5	17 15 19.0	-31 34 05.9	354.20	+4.02		5.5	S,D		-	114
078	Sa 3-43	17 17 55.9	-30 01 48.0	355.79	+4.45		7.9	S		-	54.4
079	Draco C-1	17 19 57.6	+57 50 04.9			17.0	11.4		+	+	77.5
080	Th 3-7	17 21 02.4	-29 22 59.4	356.70	+4.27	14.0	8.1	S		-	114
081	Th 3-17	17 27 31.9	-29 02 53.0	357.78	+3.27	14.0	8.2	S		-	54.4
082	Th 3-18	17 28 27.0	-28 38 34.0	358.23	+3.33	12.6	8.2	S		-	114
083	Hen 3-1410	17 29 06.0	-29 43 24.1	357.41	+2.61	12.8	8.5	S		-	114
084 $^\star$	V2116 Oph	17 32 03.0	-24 44 44.3	1.94	+4.79	19.0	8.1	S		+	235
085	Th 3-29	17 32 28.0	-29 05 06.0	358.34	+2.35	17.0	7.0	S		-	35.1
086	Th 3-30	17 33 43.0	-28 07 18.0	359.30	+2.65	13.1	8.3	S		-	114
087	Th 3-31	17 34 26.5	-29 28 05.0	358.25	+1.78	13.6	7.6	S		-	114
088 $^\star$	M 1-21	17 34 17.2	-19 09 21.9	6.96	+7.36	13.7	7.2	S		-	114
089 $^\star$	Hen 2-251	17 35 22.3	-29 45 20.0	358.12	+1.46	15.4	7.3	D		-	114
090	Pt 1	17 38 49.8	-23 54 02.9	3.48	+3.94	15.0	8.6	S		-	114
091	K 6-6	17 39 18.3	-28 15 06.9	359.85	+1.54	16.5		S		-	114
092 $^\star$	RT Ser	17 39 51.8	-11 56 44.7	13.89	+9.97	15.0	7.0	S	+	-	114
093 $^\star$	AE Ara	17 41 04.9	-47 03 20.9	344.00	-8.66	12.5	6.4	S	+	-	77.5
094 $^\star$	SS73 96	17 41 28.3	-36 47 51.9	352.85	-3.38	15.2	6.4	S		-	100
095	UU Ser	17 42 37.9	-15 24 29.9	11.23	+7.62	15.3	9.1	S		-	114
096 $^\star$	V2110 Oph	17 43 33.3	-22 45 37.0	5.03	+3.62	19	7.9	D		-	114
097	V916 Sco	17 43 54.9	-36 03 24.9	353.73	-3.41		8.3	S		-	54.4
098	Hen 2-275	17 45 31.0	-38 39 47.9	351.67	-5.03	15.5	>9.3	S		-	114
099	V917 Sco	17 48 04.0	-36 08 17.9	354.10	-4.17	13.0	7.9	S		-	114
100 $^\star$	H 1-36	17 49 48.1	-37 01 27.9	353.51	-4.92	12.0	7.5	D	+	+	114

**Table 1:** continued
No.	Cool-star spectrum	Radio	IRAS	IRAS	References
		[mJy]	F₁₂[Jy]	F₂₅[Jy]
051	K2(Mürset & Schmid 1999)	<0.22(3.6 cm)			Allen 1984 (fc,class,spc) Smith et al. 1997 (parm)
052	Mira M5/M7(Mürset & Schmid 1999,Allen 1980)	0.70(3.5 cm)	0.5	0.3	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
053	M5.5(Mürset & Schmid 1999)	10(6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
054	M3.5/M0(Mürset & Schmid 1999,Allen 1980)	<1(2 cm)			Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc,parm)
055	G5(Mürset & Schmid 1999)	34(2 cm)	20.0	37.4	Allen 1984 (fc,spc) Belczynski 2000 (class) Schmid & Nussbaumer 1993 (parm)
056	Mira,M6.5(Mürset & Schmid 1999)		4.9	2.8	Allen 1984 (fc,class,spc)
057	M4.5(Mürset & Schmid 1999)	<0.08(3.6 cm)	0.68	0.20	Allen 1984 (fc,class) Selvelli et al. 1992 (spc) Belczynski et al. 1998 (parm)
058	K2(Mürset & Schmid 1999)	0.48(6 cm)	0.25	0.09	Allen 1984 (fc,class) Blair et al. 1983 (spc) Miko $\l$ ajewska et al. 1995 (parm)
059	M6(Mürset & Schmid 1999)				Allen 1984 (fc,class)
060	Mira M7/M8.5(Mürset & Schmid 1999,Allen 1980)	<12(6 cm)	5.3	2.9	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
061	C4.5Jch(Schmid 1994)	<0.07(3.6 cm)			Allen 1984 (fc,spc,class) Schmid 1994 (parm)
062	mid M(MacConnell 1983)				Perek & Kohoutek 1967 (fc) Miko $\l$ ajewska et al. 1997 (class,spc,parm) Pereira et al. 1998 (parm)
063	M3,M6(Mürset & Schmid 1999,Medina Tanco & Steiner 1995)	<0.07(3.6 cm)			Allen 1984 (fc,class,spc)
064	Mira M6.5,M6(Mürset & Schmid 1999,Medina Tanco & Steiner 1995)	3.39(3.6 cm)	7.7	4.5	Allen 1984 (fc,class,spc) Kaler et al. 1991 (parm)
065	M2/K4(Sanduleak & Stephenson 1973,Allen 1980)	<12(6 cm)			Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc,parm)
066	M4.5,M7(Mürset & Schmid 1999,Medina Tanco & Steiner 1995)	0.21(3.6 cm)	0.20	0.05L	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
067	Mira(Whitelock 1987);M4/M7(Mürset & Schmid 1999,Allen 1980)	4.05(3.6 cm)	2.3	3.6	Allen 1984 (fc,class,spc)
068	M6(Mürset & Schmid 1999)	<22(6 cm)	0.35	0.17	Duerbeck 1987 (fc) Allen 1984 (class) Gutierrez-Moreno et al. 1999 (spc) Feibelman 1991 (parm)
069	Mira; C3(Medina Tanco & Steiner 1995)	4.56(3.6 cm)	4.0	1.2	Allen 1984 (fc,class,spc) Schmid & Nussbaumer 1993 (parm)
070	M3.5(Mürset & Schmid 1999)	<0.07(3.6 cm)			Allen 1984 (fc,class,spc)
071	M5(Mürset & Schmid 1999)	0.34(3.6 cm)	0.04L	0.18L	Allen 1984 (fc,class,spc) Michalitsianos et al. 1982 (parm)
072	M2(Miko $\l$ ajewska et al. 1997)				MacConnell 1978 (fc) Miko $\l$ ajewska et al. 1997 (spc,class,parm)
073	M6.5,M6(Mürset & Schmid 1999,Medina Tanco & Steiner 1995)	1.99(3.6 cm)	1.50	1.00	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
074	M4/M0(Mürset & Schmid 1999,Allen 1980)	1.04(3.6 cm)			Allen 1984 (fc,class,spc) Gutierrez-Moreno et al. 1997 (parm)
075	M0(Mürset & Schmid 1999)	<0.08(3.6 cm)			Allen 1984 (fc,class,spc)
076	M7.5(Mürset & Schmid 1999)	0.16(3.6 cm)	3.32	3.46	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
077	M5.5(Mürset & Schmid 1999)	<0.09(3.6 cm)	0.4	0.8L	Allen 1984 (fc,class,spc)
078	early M(Allen 1984)	<0.57(6 cm)			Allen 1984 (fc,class) Gutierrez-Moreno et al. 1992 (spc,parm)
079	C1.2(Kenyon 1986)	<0.10(3.6 cm)			Allen 1984 (fc,class) Aaronson et al. 1982 (spc) Munari & Buson 1994 (parm)
080	M5(Medina Tanco & Steiner 1995)	0.36(6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
081	M3(Miko $\l$ ajewska et al. 1997)	<0.11(3.6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
082	M3(Medina Tanco & Steiner 1995)	<0.14(3.6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
083	M1.5,M3(Mürset & Schmid 1999,Miko $\l$ ajewska et al. 1997)	0.57(6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
084	M5/M6:(Chakrabarty & Roche 1997,Allen 1980)	0.06:(6 cm)			Davidsen et al. 1977 (spc,class) Chakrabarty & Roche 1997 (fc,parm)
085	M3(Miko $\l$ ajewska et al. 1997)	<0.26(6 cm)	6.02	5.62	Acker et al. 1988 (fc,class) Miko $\l$ ajewska et al. 1997 (spc,parm)
086	M1(Miko $\l$ ajewska et al. 1997)	<0.11(3.6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
087	M5(Allen 1980)	<0.10(3.6 cm)	1.89	2.10	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
088	M6/M2(Mürset & Schmid 1999,Allen 1980)	0.51(3.6 cm)	0.65	0.36:	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
089	late M(Miko $\l$ ajewska et al. 2000)		7.33	7.46	Perek & Kohoutek 1967 (fc) Cieslinski et al. 1994 (spc) Miko $\l$ ajewska et al. 1997 (class,parm)
090	M3(Mürset & Schmid 1999)	<0.10(3.6 cm)			Allen 1984 (fc,class,spc) Munari et al. 1994 (parm)
091					Kohoutek 1994 (fc) Lundstrom & Stenholm 1984 (spc) Miko $\l$ ajewska et al. 1997 (class,parm)
092	M6(Mürset & Schmid 1999)	1.19(3.6 cm)	0.12	0.05L	Allen 1984 (fc,class,spc) Shugarov et al. 1997 (parm)
093	M5.5/M2(Mürset & Schmid 1999,Allen 1980)	<18(2 cm)	0.22	0.08L	Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc) Miko $\l$ ajewska et al. 2000 (parm)
094	M0/M2(Medina Tanco & Steiner 1995,Allen 1980)	1.59(3.6 cm)	0.43	0.35L	Allen 1984 (fc,class,spc)
095	M4(Miko $\l$ ajewska et al. 1997)	<0.13(3.6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
096	Mira M8(Allen 1980)	<0.19(3.6 cm)	0.15	0.06L	Allen 1984 (fc,class,spc)
097	M(Kenyon 1986)	<0.14(3.6 cm)			Allen 1984 (fc,class) Sanduleak et al. 1978 (parm)
098	M3(Miko $\l$ ajewska et al. 1997)				Acker et al. 1988 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
099	M7(Allen 1980)	<0.12(3.6 cm)			Allen 1984 (fc,class,spc)
100	Mira(Allen 1983);M4-5:(Medina Tanco & Steiner 1995)	65.3(3.6 cm)	17.9	30.4	Allen 1984 (fc,class,spc) Pereira et al. 1998 (parm)

Table 1: continued
No. Name $\alpha$ (2000) $\delta$ (2000) $l^{\rm II}$ $b^{\rm II}$ V K IR IUE X IP $_{\rm max}$

$^{\rm h}$ $^{\rm m}$ $^{\rm s}$ $^\circ$ ' '' $^\circ$ $^\circ$ [mag] [mag] [eV]

101 $^\star$ RS Oph 17 50 13.2 -06 42 28.4 19.80 +10.37 11.5 6.5 S + + 114

102 $^\star$ WRAY 16-312 17 50 16.5 -30 57 41.1 358.79 -1.91 7.8 D + 108.8

103 $^\star$ V4141 Sgr 17 50 24.0 -19 53 42.0 8.31 +3.73 16.4 7.9 D,S - 54.4

104 ALS 2 17 50 51.1 -17 47 56.0 10.18 +4.70 14.2 S 114

105 $^\star$ AS 245 17 51 00.8 -22 19 41.3 6.29 +2.38 11.0 7.2 S,D - 114

106 Hen 2-294 17 51 38.2 -32 50 57.0 357.31 -3.12 8.4 S - 114

107 $^\star$ Bl 3-14 17 52 25.9 -29 46 00.0 0.05 -1.70 14.3 8.7 S - 114

108 Bl 3-6 17 52 57.0 -31 19 18.0 358.77 -2.59 17.0 S - 114

109 Bl L 17 53 13.0 -30 18 00.0 359.68 -2.12 16.0 7.8 S - 114

110 $^\star$ V745 Sco 17 55 22.2 -33 14 59.3 357.36 -4.00 17 8.4 S + - 262

111 MaC 1-9 17 55 52.6 -14 06 49.3 13.99 +5.51 15.2 S - 54.4

112 $^\star$ AS 255 17 57 08.7 -35 15 38.0 355.79 -5.32 12.5 8.4 S,D - 114

113 V2416 Sgr 17 57 15.9 -21 41 35.4 7.57 +1.44 15.1 4.6 S + - 114

114 $^\star$ H 2-34 17 58 28.0 -28 33 42.0 1.76 -2.23 18.0 >9.9 - 114

115 $^\star$ SS73 117 18 02 22.9 -31 59 11.0 359.19 -4.66 12.5 7.7 S - 114

116 $^\star$ AS 269 18 03 23.8 -32 42 21.9 358.67 -5.20 13.9 8.7 D' - 54.4

117 Ap 1-8 18 04 29.8 -28 21 28.0 2.59 -3.28 15.2 7.9 S - 114

118 $^\star$ SS73 122 18 04 41.1 -27 09 32.8 3.66 -2.73 12.0 6.6 D - 114

119 AS 270 18 05 33.6 -20 20 44.6 9.64 +0.37 13.1 5.5 S - 54.4

120 $^\star$ H 2-38 18 06 01.0 -28 17 10.8 2.81 -3.54 13.8 6.7 D + + 114

121 SS73 129 18 07 05.7 -29 36 25.9 1.77 -4.39 12.5 8.0 S - 114

122 $^\star$ Hen 3-1591 18 07 31.9 -25 53 44.0 5.07 -2.68 12.5 9.0 S,D' + 54.4

123 V615 Sgr 18 07 49.6 -36 10 09.0 356.05 -7.66 13.3 7.6 S - 54.4

124 $^\star$ Ve 2-57 18 08 24.0 -24 34 00.0 6.33 -2.20 12.5 7.4 S - 35.1

125 $^\star$ AS 276 18 09 09.6 -41 13 26.0 351.64 -10.24 12.0 8.1 S,D - 114

126 Ap 1-9 18 10 28.9 -28 07 41.0 3.43 -4.33 12.5 8.8 S - 54.4

127 AS 281 18 10 47.5 -27 56 24.0 3.63 -4.30 12.9 7.0 S - 114

128 $^\star$ V2506 Sgr 18 11 01.6 -28 32 39.9 3.12 -4.63 12.0 8.4 S - 114

129 SS73 141 18 12 11.2 -33 10 41.0 359.13 -7.04 12.5 9.0 S - 54.4

130 AS 289 18 12 22.0 -11 40 13.0 18.08 +3.20 12.1 5.0 S + - 114

131 Y CrA 18 14 24.1 -42 51 00.0 350.60 -11.84 14.4 6.6 S + - 114

132 $^\star$ YY Her 18 14 34.3 +20 59 20.0 48.14 +17.24 12.8 8.0 S + - 109.3

133 $^\star$ V2756 Sgr 18 14 34.5 -29 49 22.4 2.36 -5.92 11.5 7.8 S - 114

134 $^\star$ FG Ser 18 15 06.2 -00 18 57.6 28.5 +7.9 11.0 4.5 S + - 100

135 HD 319167 18 15 24.5 -30 31 57.2 1.81 -6.41 12.5 7.5 S - 54.4

136 Hen 2-374 18 15 36.4 -21 34 40.0 9.75 -2.23 12.0 6.5 S - 114

137 Hen 2-376 18 15 46.0 -27 53 48.0 4.19 -5.24 14.1 S + 35.1

138 $^\star$ V4074 Sgr 18 16 05.5 -30 51 11.3 1.59 -6.69 11.5 7.7 + - 235

139 $^\star$ V2905 Sgr 18 17 20.5 -28 09 51.0 4.11 -5.68 12.3 7.1 S - 63.5

140 StHA 149 18 18 55.9 +27 26 12.0 54.81 +18.77 13.5 114

141 Hen 3-1674 18 20 19.2 -26 22 47.8 6.01 -5.43 12.5 7.7 S - 114

142 AR Pav 18 20 27.8 -66 04 42.9 328.54 -21.60 10.0 7.2 S + - 97.1

143 V3929 Sgr 18 20 58.8 -26 48 32.0 5.70 -5.76 12 7.4 D - 114

144 V3804 Sgr 18 21 28.5 -31 32 03.9 1.52 -8.02 12.0 7.3 S - 114

145 V443 Her 18 22 08.4 +23 27 20.0 51.23 +16.59 11.5 5.4 S + - 97.1

146 $^\star$ V3811 Sgr 18 23 28.9 -21 53 08.9 10.34 -3.98 14 8.5 S - 54.4

147 V4018 Sgr 18 25 27.0 -28 35 57.5 4.55 -7.46 11.4 7.5 S + - 100

148 $^\star$ V3890 Sgr 18 30 43.0 -24 00 59.0 9.21 -6.44 $\sim$ 14 8.2 S + 361

149 V2601 Sgr 18 37 58.9 -22 42 07.9 11.14 -7.34 15 8.0 S - 54.4

150 K 3-9 18 40 24.1 -08 43 46.6 23.91 -1.54 18.0 5.6 D - 114

**Table 1:** continued
No.	Name	$\alpha$ (2000)	$\delta$ (2000)	$l^{\rm II}$	$b^{\rm II}$	V	K	IR	IUE	X	IP $_{\rm max}$
		$^{\rm h}$ $^{\rm m}$ $^{\rm s}$	$^\circ$ ' ''	$^\circ$	$^\circ$	[mag]	[mag]				[eV]
101 $^\star$	RS Oph	17 50 13.2	-06 42 28.4	19.80	+10.37	11.5	6.5	S	+	+	114
102 $^\star$	WRAY 16-312	17 50 16.5	-30 57 41.1	358.79	-1.91		7.8	D		+	108.8
103 $^\star$	V4141 Sgr	17 50 24.0	-19 53 42.0	8.31	+3.73	16.4	7.9	D,S		-	54.4
104	ALS 2	17 50 51.1	-17 47 56.0	10.18	+4.70	14.2		S			114
105 $^\star$	AS 245	17 51 00.8	-22 19 41.3	6.29	+2.38	11.0	7.2	S,D		-	114
106	Hen 2-294	17 51 38.2	-32 50 57.0	357.31	-3.12		8.4	S		-	114
107 $^\star$	Bl 3-14	17 52 25.9	-29 46 00.0	0.05	-1.70	14.3	8.7	S		-	114
108	Bl 3-6	17 52 57.0	-31 19 18.0	358.77	-2.59	17.0		S		-	114
109	Bl L	17 53 13.0	-30 18 00.0	359.68	-2.12	16.0	7.8	S		-	114
110 $^\star$	V745 Sco	17 55 22.2	-33 14 59.3	357.36	-4.00	17	8.4	S	+	-	262
111	MaC 1-9	17 55 52.6	-14 06 49.3	13.99	+5.51	15.2		S		-	54.4
112 $^\star$	AS 255	17 57 08.7	-35 15 38.0	355.79	-5.32	12.5	8.4	S,D		-	114
113	V2416 Sgr	17 57 15.9	-21 41 35.4	7.57	+1.44	15.1	4.6	S	+	-	114
114 $^\star$	H 2-34	17 58 28.0	-28 33 42.0	1.76	-2.23	18.0	>9.9			-	114
115 $^\star$	SS73 117	18 02 22.9	-31 59 11.0	359.19	-4.66	12.5	7.7	S		-	114
116 $^\star$	AS 269	18 03 23.8	-32 42 21.9	358.67	-5.20	13.9	8.7	D'		-	54.4
117	Ap 1-8	18 04 29.8	-28 21 28.0	2.59	-3.28	15.2	7.9	S		-	114
118 $^\star$	SS73 122	18 04 41.1	-27 09 32.8	3.66	-2.73	12.0	6.6	D		-	114
119	AS 270	18 05 33.6	-20 20 44.6	9.64	+0.37	13.1	5.5	S		-	54.4
120 $^\star$	H 2-38	18 06 01.0	-28 17 10.8	2.81	-3.54	13.8	6.7	D	+	+	114
121	SS73 129	18 07 05.7	-29 36 25.9	1.77	-4.39	12.5	8.0	S		-	114
122 $^\star$	Hen 3-1591	18 07 31.9	-25 53 44.0	5.07	-2.68	12.5	9.0	S,D'		+	54.4
123	V615 Sgr	18 07 49.6	-36 10 09.0	356.05	-7.66	13.3	7.6	S		-	54.4
124 $^\star$	Ve 2-57	18 08 24.0	-24 34 00.0	6.33	-2.20	12.5	7.4	S		-	35.1
125 $^\star$	AS 276	18 09 09.6	-41 13 26.0	351.64	-10.24	12.0	8.1	S,D		-	114
126	Ap 1-9	18 10 28.9	-28 07 41.0	3.43	-4.33	12.5	8.8	S		-	54.4
127	AS 281	18 10 47.5	-27 56 24.0	3.63	-4.30	12.9	7.0	S		-	114
128 $^\star$	V2506 Sgr	18 11 01.6	-28 32 39.9	3.12	-4.63	12.0	8.4	S		-	114
129	SS73 141	18 12 11.2	-33 10 41.0	359.13	-7.04	12.5	9.0	S		-	54.4
130	AS 289	18 12 22.0	-11 40 13.0	18.08	+3.20	12.1	5.0	S	+	-	114
131	Y CrA	18 14 24.1	-42 51 00.0	350.60	-11.84	14.4	6.6	S	+	-	114
132 $^\star$	YY Her	18 14 34.3	+20 59 20.0	48.14	+17.24	12.8	8.0	S	+	-	109.3
133 $^\star$	V2756 Sgr	18 14 34.5	-29 49 22.4	2.36	-5.92	11.5	7.8	S		-	114
134 $^\star$	FG Ser	18 15 06.2	-00 18 57.6	28.5	+7.9	11.0	4.5	S	+	-	100
135	HD 319167	18 15 24.5	-30 31 57.2	1.81	-6.41	12.5	7.5	S		-	54.4
136	Hen 2-374	18 15 36.4	-21 34 40.0	9.75	-2.23	12.0	6.5	S		-	114
137	Hen 2-376	18 15 46.0	-27 53 48.0	4.19	-5.24	14.1		S	+		35.1
138 $^\star$	V4074 Sgr	18 16 05.5	-30 51 11.3	1.59	-6.69	11.5	7.7		+	-	235
139 $^\star$	V2905 Sgr	18 17 20.5	-28 09 51.0	4.11	-5.68	12.3	7.1	S		-	63.5
140	StHA 149	18 18 55.9	+27 26 12.0	54.81	+18.77	13.5					114
141	Hen 3-1674	18 20 19.2	-26 22 47.8	6.01	-5.43	12.5	7.7	S		-	114
142	AR Pav	18 20 27.8	-66 04 42.9	328.54	-21.60	10.0	7.2	S	+	-	97.1
143	V3929 Sgr	18 20 58.8	-26 48 32.0	5.70	-5.76	12	7.4	D		-	114
144	V3804 Sgr	18 21 28.5	-31 32 03.9	1.52	-8.02	12.0	7.3	S		-	114
145	V443 Her	18 22 08.4	+23 27 20.0	51.23	+16.59	11.5	5.4	S	+	-	97.1
146 $^\star$	V3811 Sgr	18 23 28.9	-21 53 08.9	10.34	-3.98	14	8.5	S		-	54.4
147	V4018 Sgr	18 25 27.0	-28 35 57.5	4.55	-7.46	11.4	7.5	S	+	-	100
148 $^\star$	V3890 Sgr	18 30 43.0	-24 00 59.0	9.21	-6.44	$\sim$ 14	8.2	S	+		361
149	V2601 Sgr	18 37 58.9	-22 42 07.9	11.14	-7.34	15	8.0	S		-	54.4
150	K 3-9	18 40 24.1	-08 43 46.6	23.91	-1.54	18.0	5.6	D		-	114

**Table 1:** continued
No.	Cool-star spectrum	Radio	IRAS	IRAS	References
		[mJy]	F₁₂[Jy]	F₂₅[Jy]
101	M0-M2(Dobrzycka et al. 1996,Anupama et al. 1999)	<0.33(3.6 cm)	0.30	0.16	Allen 1984 (fc,class,spc) Dobrzycka et al. 1996,Bode 1987 (parm)
102	Mira(Whitelock 1988)	0.96(6 cm)	5.0	3.1	Allen 1984 (fc,spc) Belczynski 2000 (class)
103	M6(Miko $\l$ ajewska et al. 2000)	<0.17(6 cm)	1.88	0.65	Allen 1984 (fc) Gutierrez-Moreno et al. 1992 (spc,class) Miko $\l$ ajewska et al. 1997 (spc,parm)
104	M2(Miko $\l$ ajewska et al. 1997)				Acker et al. 1988 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
105	Mira(Whitelock 1988);M6(Allen 1980)	0.87(6 cm)	1.67	0.62	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
106	M3(Miko $\l$ ajewska et al. 1997)	<0.11(3.6 cm)	2.19	2.89	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
107	M6(Gutierrez-Moreno & Moreno 1995)	<0.12(3.6 cm)			Allen 1984 (fc,class,spc) Gutierrez-Moreno & Moreno 1995 (parm)
108	M3(Miko $\l$ ajewska et al. 1997)	<0.20(6 cm)	1.62	1.14	Acker et al. 1988 (fc,class) Miko $\l$ ajewska et al. 1997 (spc,parm)
109	M6.5(Allen 1980)	<0.10(3.6 cm)			Allen 1984 (fc,class,spc)
110	M6,M7(Anupama et al. 1999,Sekiguchi et al. 1990)				Sekiguchi et al. 1990 (fc) Williams et al. 1994 (spc,class) Anupama et al. 1999 (parm)
111	M2(Miko $\l$ ajewska et al. 1997)				MacConnell 1978 (fc) Miko $\l$ ajewska et al. 1997 (spc,class,parm)
112	K3(Medina Tanco & Steiner 1995)	<0.10(3.6 cm)	1.31L	1.58L	Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc,parm)
113	M6/M5(Mürset & Schmid 1999,Allen 1980)	2.26(3.6 cm)	1.44	0.71	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
114	M5:(Belczynski 2000)				185(fc) Acker et al. 1988 (spc,class)
115	M5/M6(Medina Tanco & Steiner 1995,Allen 1980)	0.25(3.6 cm)	0.33	0.09	Allen 1984 (fc,class,spc)
116	G5-K2(Miko $\l$ ajewska et al. 1997)	<1(2 cm)	1.01	2.54	Perek & Kohoutek 1967 (fc) Belczynski 2000 (class) Miko $\l$ ajewska et al. 1997 (spc)
117	M4/M0(Miko $\l$ ajewska et al. 1997,Allen 1980)	<0.10(3.6 cm)	0.66	0.49	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
118	Mira(Whitelock 1988);M7(Medina Tanco & Steiner 1995)	2.19(3.6 cm)	1.4	1.2	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
119	M5.5/M1(Mürset & Schmid 1999,Allen 1980)	0.29(3.6 cm)	1.67	5.98L	Allen 1984 (fc,class,spc) Gutierrez-Moreno et al. 1999 (spc,parm)
120	Mira(Whitelock 1988);M7(Mürset & Schmid 1999)	4.50(3.6 cm)	3.2	2.0	Allen 1984 (fc,class) Pereira et al. 1998 (spc,parm)
121	M0(Mürset & Schmid 1999)	<0.14(3.6 cm)	0.74	1.42L	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
122	G(Allen 1980)	0.41(3.6 cm)	1.0	0.6	Allen 1984 (fc,class,spc) Gutierrez-Moreno & Moreno 1996 (parm)
123	M5.5,M5(Mürset & Schmid 1999,Medina Tanco & Steiner 1995)	<0.11(3.6 cm)	0.87	0.54L	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
124	M(Allen 1978)	<0.25(6 cm)			Allen 1984 (fc,spc) Belczynski 2000 (class)
125	M4.5(Mürset & Schmid 1999)	<0.14(3.6 cm)	0.31L	0.37L	Allen 1984 (fc,class,spc)
126	K5/K4(Miko $\l$ ajewska et al. 1997,Allen 1980)	<0.16(3.6 cm)	1.13	0.70:	Allen 1984 (fc,class,spc) Kaler et al. 1991 (parm)
127	M5(Medina Tanco & Steiner 1995)	0.24(3.6 cm)	0.79	0.54:	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
128	M5.5(Mürset & Schmid 1999)	0.23(3.6 cm)	0.21	0.18L	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
129	M5(Mürset & Schmid 1999)	<0.10(3.6 cm)			Allen 1984 (fc,class,spc)
130	M3.5(Mürset & Schmid 1999)	1.84(3.6 cm)	0.55	0.45L	Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc,parm)
131	M6/M5(Mürset & Schmid 1999,Allen 1980)	0.31(3.6 cm)	0.25L	0.25L	Allen 1984 (fc,class) Gutierrez-Moreno et al. 1999 (spc,parm)
132	M4(Mürset & Schmid 1999)	<0.11(3.6 cm)	0.10	0.04L	Allen 1984 (fc,class,spc) Munari et al. 1997 (parm)
133	M3(Medina Tanco & Steiner 1995)	0.17(3.6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
134	M5.3,M5(Kenyon & Fernandez-Castro 1987,Mürset & Schmid 1999)	0.43(6 cm)	1.00	0.35	Allen 1984 (fc,class,spc) Mürset et al. 2000 (parm)
135	M3(Miko $\l$ ajewska et al. 1997,Medina Tanco & Steiner 1995)	0.31(3.6 cm)			Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
136	M5.5(Mürset & Schmid 1999)	0.39(3.6 cm)	1.28	0.71:	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
137	M2(Miko $\l$ ajewska et al. 1997)				Acker et al. 1988 (fc) Cieslinski et al. 1994,Miko $\l$ ajewska et al. 1997 (spc,class) Miko $\l$ ajewska et al. 1997 (parm)
138	M4(Munari 1997)	<0.47(3.6 cm)	14.6	65.1	Allen 1984 (fc,class,spc) Munari 1997 (parm)
139	late M,M0(Allen 1975,Miko $\l$ ajewska et al. 1997)		0.07L	0.06L	Miko $\l$ ajewska et al. 1997 (class,parm) Pereira et al. 1998 (spc)
140	M2(Stephenson 1986)				Downes & Keyes 1988 (spc,class)
141	M5(Medina Tanco & Steiner 1995)	0.28(3.6 cm)			Allen 1984 (fc,class,spc)
142	M5/M6(Mürset & Schmid 1999,Allen 1980)	<14(6 cm)	0.14	0.05L	Allen 1984 (fc,class,spc) Schild et al. 2000 (parm)
143	Mira M1-2(Medina Tanco & Steiner 1995)	0.28(3.6 cm)	5.0	4.1	Allen 1984 (fc,class,spc) Remillard et al. 1992 (parm)
144	M5/M6(Medina Tanco & Steiner 1995,Allen 1980)	0.46(3.6 cm)	0.52	0.26	Allen 1984 (fc) Pereira et al. 1998 (spc) Kenyon 1986 (class) Gutierrez-Moreno et al. 1992 (parm)
145	M5.5(Mürset & Schmid 1999)	0.23(3.6 cm)	0.40	0.13	Allen 1984 (fc,class,spc) Dobrzycka et al. 1993 (parm)
146	M3.5(Mürset & Schmid 1999)	<0.07(3.6 cm)	5.40	2.20	Allen 1984 (fc,class,spc)
147	M4(Allen 1980)	<0.11(3.6 cm)	0.44	0.27L	Allen 1984 (fc,class) Allen 1984,Gutierrez-Moreno et al. 1999 (spc) Munari & Buson 1993 (parm)
148	M5,M8(Harrison et al. 1993,Williams et al. 1991)				Duerbeck 1987 (fc) Williams et al. 1991 (spc) Belczynski 2000 (class) Anupama et al. 1999 (parm)
149	M5(Miko $\l$ ajewska et al. 1997)	<0.12(3.6 cm)	0.50	0.50L	Allen 1984 (fc,class,spc) Miko $\l$ ajewska et al. 1997 (spc,parm)
150	Mira(Ivison & Seaquist 1995,Miko $\l$ ajewska et al. 1997);M3(Miko $\l$ ajewska et al. 1997)	8.63(3.6 cm)	8.09	4.08	Perek & Kohoutek 1967 (fc) Miko $\l$ ajewska et al. 1997 (spc,class) Ivison & Seaquist 1995,Miko $\l$ ajewska et al. 1997 (parm)

Table 1: continued
No. Name $\alpha$ (2000) $\delta$ (2000) $l^{\rm II}$ $b^{\rm II}$ V K IR IUE X IP $_{\rm max}$

$^{\rm h}$ $^{\rm m}$ $^{\rm s}$ $^\circ$ ' '' $^\circ$ $^\circ$ [mag] [mag] [eV]

151 AS 316 18 42 33.0 -21 17 48.0 12.89 -7.67 12.0 7.8 S - 114

152 DQ Ser 18 44 40.0 +05 03 29.9 36.67 +3.81 14.6 54.4

153 MWC 960 18 47 55.9 -20 05 49.9 14.53 -8.27 12.0 7.8 S + - 114

154 AS 323 18 48 35.7 -06 41 08.9 26.66 -2.41 15.5 7.9 S - 114

155 AS 327 18 53 16.9 -24 22 54.0 11.14 -11.23 11.8 8.5 S - 114

156 $^\star$ FN Sgr 18 53 52.9 -18 59 42.0 16.15 -9.06 12.7 7.9 S + - 114

157 Pe 2-16 18 54 10.0 -04 38 53.9 29.10 -2.72 16.0 8.1 S - 114

158 CM Aql 19 03 35.2 -03 03 15.0 31.59 -4.09 13.6 7.7 S - 54.4

159 V919 Sgr 19 03 46.0 -16 59 53.9 19.01 -10.32 12.2 7.3 S - 54.4

160 $^\star$ V1413 Aql 19 03 51.6 +16 28 31.7 48.97 +4.77 14.0 7.5 S + - 114

161 NSV 11776 19 09 55.8 -02 47 40.3 32.55 -5.39 13.6 114

162 $^\star$ Ap 3-1 19 10 36.1 +02 49 32.0 37.64 -2.97 15.4 8.6 S +? 114

163 MaC 1-17 19 12 57.3 -05 21 20.0 30.59 -7.22 15.6 S - 63.5

164 V352 Aql 19 13 33.6 +02 18 14.0 37.51 -3.86 16.2 >9.6 S - 114

165 ALS 1 19 16 16.2 -08 17 45.9 28.30 -9.27 14.8 S 114

166 $^\star$ BF Cyg 19 23 53.4 +29 40 25.1 62.93 +6.70 12.3 6.3 S + - 97.1

167 $^\star$ CH Cyg 19 24 33.0 +50 14 29.1 81.86 +15.58 7.1 -0.7 S + + 77.5

168 StHA 164 19 28 40.9 -06 03 42.0 31.73 -11.03 13.6 114

169 $^\star$ HM Sge 19 41 57.1 +16 44 39.9 53.57 -3.15 17 4.3 D + + 205.1

170 $^\star$ Hen 3-1761 19 42 25.3 -68 07 35.3 327.67 -29.76 10.4 5.6 S + - 100

171 $^\star$ QW Sge 19 45 49.6 +18 36 50.0 55.64 -3.02 12.8 7.1 S + - 114

172 $^\star$ CI Cyg 19 50 11.8 +35 41 03.2 70.90 +4.74 11.0 4.5 S + - 109.3

173 StHA 169 19 51 28.9 +46 23 06.0 80.38 +9.85 >13.5 54.4

174 $^\star$ V1016 Cyg 19 57 04.9 +39 49 33.9 75.17 +5.68 11.2 5.3 D + + 141.3

175 RR Tel 20 04 18.5 -55 43 33.1 342.16 -32.24 10.8 4.2 D + + 141.3

176 $^\star$ PU Vul 20 21 12.0 +21 34 41.9 62.58 -8.52 11.6 6.2 S + + 235

177 $^\star$ LT Del 20 35 57.3 +20 11 34.0 63.40 -12.15 13.1 9.4 S + - 77.5

178 StHA 180 20 39 21.0 -05 16 59.9 40.89 -26.36 13.5 114

179 Hen 2-468 20 41 18.9 +34 44 52.0 75.94 -4.44 14.2 8.0 S - 114

180 $^\star$ ER Del 20 42 46.4 +08 40 56.4 54.46 -20.00 10 + - 47.9

181 $^\star$ V1329 Cyg 20 51 01.1 +35 34 51.2 77.80 -5.56 13.3 6.9 S + - 141.3

182 CD-43 14304 21 00 06.3 -42 38 49.9 358.65 -41.10 10.8 7.6 S + + 114

183 $^\star$ V407 Cyg 21 02 13.0 +45 46 30.0 86.99 -0.49 14 3.3 D + - 54.4

184 $^\star$ StHA 190 21 41 44.8 +02 43 54.4 58.41 -35.43 10.5 7.8 D' + - 47.9

185 $^\star$ AG Peg 21 51 01.9 +12 37 29.4 69.28 -30.89 9.0 3.9 S + + 100

186 $^\star$ LL Cas 23 09 20.1 +54 44 53.0 108.47 -5.23 15 7.6 S 54.4:

187 $^\star$ Z And 23 33 39.5 +48 49 05.4 109.98 -12.09 10.8 5.0 S + + 114

188 $^\star$ R Aqr 23 43 49.4 -15 17 04.2 66.52 -70.33 9.1 -0.9 D + + 97.1

**Table 1:** continued
No.	Name	$\alpha$ (2000)	$\delta$ (2000)	$l^{\rm II}$	$b^{\rm II}$	V	K	IR	IUE	X	IP $_{\rm max}$
		$^{\rm h}$ $^{\rm m}$ $^{\rm s}$	$^\circ$ ' ''	$^\circ$	$^\circ$	[mag]	[mag]				[eV]
151	AS 316	18 42 33.0	-21 17 48.0	12.89	-7.67	12.0	7.8	S		-	114
152	DQ Ser	18 44 40.0	+05 03 29.9	36.67	+3.81	14.6					54.4
153	MWC 960	18 47 55.9	-20 05 49.9	14.53	-8.27	12.0	7.8	S	+	-	114
154	AS 323	18 48 35.7	-06 41 08.9	26.66	-2.41	15.5	7.9	S		-	114
155	AS 327	18 53 16.9	-24 22 54.0	11.14	-11.23	11.8	8.5	S		-	114
156 $^\star$	FN Sgr	18 53 52.9	-18 59 42.0	16.15	-9.06	12.7	7.9	S	+	-	114
157	Pe 2-16	18 54 10.0	-04 38 53.9	29.10	-2.72	16.0	8.1	S		-	114
158	CM Aql	19 03 35.2	-03 03 15.0	31.59	-4.09	13.6	7.7	S		-	54.4
159	V919 Sgr	19 03 46.0	-16 59 53.9	19.01	-10.32	12.2	7.3	S		-	54.4
160 $^\star$	V1413 Aql	19 03 51.6	+16 28 31.7	48.97	+4.77	14.0	7.5	S	+	-	114
161	NSV 11776	19 09 55.8	-02 47 40.3	32.55	-5.39	13.6					114
162 $^\star$	Ap 3-1	19 10 36.1	+02 49 32.0	37.64	-2.97	15.4	8.6	S		+?	114
163	MaC 1-17	19 12 57.3	-05 21 20.0	30.59	-7.22	15.6		S		-	63.5
164	V352 Aql	19 13 33.6	+02 18 14.0	37.51	-3.86	16.2	>9.6	S		-	114
165	ALS 1	19 16 16.2	-08 17 45.9	28.30	-9.27	14.8		S			114
166 $^\star$	BF Cyg	19 23 53.4	+29 40 25.1	62.93	+6.70	12.3	6.3	S	+	-	97.1
167 $^\star$	CH Cyg	19 24 33.0	+50 14 29.1	81.86	+15.58	7.1	-0.7	S	+	+	77.5
168	StHA 164	19 28 40.9	-06 03 42.0	31.73	-11.03	13.6					114
169 $^\star$	HM Sge	19 41 57.1	+16 44 39.9	53.57	-3.15	17	4.3	D	+	+	205.1
170 $^\star$	Hen 3-1761	19 42 25.3	-68 07 35.3	327.67	-29.76	10.4	5.6	S	+	-	100
171 $^\star$	QW Sge	19 45 49.6	+18 36 50.0	55.64	-3.02	12.8	7.1	S	+	-	114
172 $^\star$	CI Cyg	19 50 11.8	+35 41 03.2	70.90	+4.74	11.0	4.5	S	+	-	109.3
173	StHA 169	19 51 28.9	+46 23 06.0	80.38	+9.85	>13.5					54.4
174 $^\star$	V1016 Cyg	19 57 04.9	+39 49 33.9	75.17	+5.68	11.2	5.3	D	+	+	141.3
175	RR Tel	20 04 18.5	-55 43 33.1	342.16	-32.24	10.8	4.2	D	+	+	141.3
176 $^\star$	PU Vul	20 21 12.0	+21 34 41.9	62.58	-8.52	11.6	6.2	S	+	+	235
177 $^\star$	LT Del	20 35 57.3	+20 11 34.0	63.40	-12.15	13.1	9.4	S	+	-	77.5
178	StHA 180	20 39 21.0	-05 16 59.9	40.89	-26.36	13.5					114
179	Hen 2-468	20 41 18.9	+34 44 52.0	75.94	-4.44	14.2	8.0	S		-	114
180 $^\star$	ER Del	20 42 46.4	+08 40 56.4	54.46	-20.00	10			+	-	47.9
181 $^\star$	V1329 Cyg	20 51 01.1	+35 34 51.2	77.80	-5.56	13.3	6.9	S	+	-	141.3
182	CD-43 14304	21 00 06.3	-42 38 49.9	358.65	-41.10	10.8	7.6	S	+	+	114
183 $^\star$	V407 Cyg	21 02 13.0	+45 46 30.0	86.99	-0.49	14	3.3	D	+	-	54.4
184 $^\star$	StHA 190	21 41 44.8	+02 43 54.4	58.41	-35.43	10.5	7.8	D'	+	-	47.9
185 $^\star$	AG Peg	21 51 01.9	+12 37 29.4	69.28	-30.89	9.0	3.9	S	+	+	100
186 $^\star$	LL Cas	23 09 20.1	+54 44 53.0	108.47	-5.23	15	7.6	S			54.4:
187 $^\star$	Z And	23 33 39.5	+48 49 05.4	109.98	-12.09	10.8	5.0	S	+	+	114
188 $^\star$	R Aqr	23 43 49.4	-15 17 04.2	66.52	-70.33	9.1	-0.9	D	+	+	97.1

Table 1. continued

Table 2. Suspected symbiotic stars

No. Name $\alpha$ (2000) $\delta$ (2000) $l^{\rm II}$ $b^{\rm II}$ V K IR IUE X IP $_{\rm max}$

$^{\rm h}$ $^{\rm m}$ $^{\rm s}$ $^\circ$ ' '' $^\circ$ $^\circ$ [mag] [mag] [eV]

s01 $^\star$ RAW 1691 01 18 36.1 -72 42 24.0 15.3 12 - 13.6

s02 $^\star$ [BE74] 583 05 26 54.0 -71 06 00.0 16.1 13.6

s03 $^\star$ StHA 55 05 46 42.0 +06 43 48.0 199.34 -11.12 13.5 13.6

s04 $^\star$ CD-28 3719 07 01 09.4 -29 06 25.9 240.19 -10.89 10.6 5.0 13.6

s05 $^\star$ GH Gem 07 04 04.9 +12 02 12.0 203.57 +8.23 14.6 >9.7 -

s06 $^\star$ ZZ CMi 07 24 13.9 +08 53 51.7 208.64 +11.30 9.9 2.8 S 35.1

s07 $^\star$ NQ Gem 07 31 54.5 +24 30 12.5 194.63 +19.35 7.9 3.0 + - 54.4

s08 $^\star$ WRAY 16-51 09 33 29.4 -46 34 49.0 271.35 +3.80 4.4 13.6

s09 $^\star$ Hen 3-653 11 25 32.5 -59 56 31.9 292.36 +1.16 12.5 5.4 S - 29.6

s10 $^\star$ NSV 05572 12 21 52.5 -13 53 09.9 292.10 +48.36 15 13.6

s11 $^\star$ CD-27 8661 12 24 34.3 -28 19 09.0 295.78 +34.18 10.5 4.1 13.6

s12 $^\star$ AE Cir 14 44 52.0 -69 23 35.9 312.67 -8.69 14.1 54.4

s13 $^\star$ V748 Cen 14 59 37.0 -33 25 23.9 331.51 +22.24 12.6 8.1 - 13.6

s14 $^\star$ V345 Nor 16 06 44.3 -52 02 30.1 330.51 +0.05 11.4 - 13.6

s15 $^\star$ V934 Her 17 06 34.5 +23 58 18.5 45.15 +32.99 7.8 3.3 + + 77.5

s16 $^\star$ Hen 3-1383 17 20 31.5 -33 09 55.7 353.53 +2.20 12.5 - 24.6

s17 $^\star$ V503 Her 17 36 46.0 +23 18 18.0 47.00 +26.23 13.8 -

s18 $^\star$ WSTB 19W032 17 39 02.8 -28 56 35.0 359.24 +1.22 17.2 35.1

s19 $^\star$ WRAY 16-294 17 39 13.9 -25 38 06.0 2.06 +2.94 15.5 S 35.1

s20 $^\star$ AS 241 17 44 58.0 -38 18 12.9 351.92 -4.76 12.0 7.8 S - 24.6

s21 $^\star$ DT Ser 18 01 52.0 -01 26 06.0 25.92 +10.34 15.4 54.4

s22 $^\star$ V618 Sgr 18 07 57.0 -36 29 35.9 355.77 -7.83 15.2 13.6

s23 $^\star$ AS 280 18 09 52.9 -33 19 41.9 358.77 -6.69 13.2 >9.4 S 54.4

s24 $^\star$ AS 288 18 12 48.0 -28 20 00.9 3.49 -4.87 8.4 D? 54.4

s25 $^\star$ Hen 2-379 18 16 17.4 -27 04 32.9 4.97 -4.96 12.5 9.3 35.1

s26 $^\star$ V335 Vul 19 23 14.2 +24 27 40.2 58.22 +4.40 11.8 13.6

s27 $^\star$ V850 Aql 19 23 34.6 +00 38 03.0 37.18 -6.85 5.0 S 13.6

s28 $^\star$ Hen 2-442 19 39 39.0 +26 30 42.0 61.80 +2.13 14 5.3 100

s29 $^\star$ IRAS 19558+3333 19 57 48.4 +33 41 15.9 69.98 +2.38 D?

s30 $^\star$ V627 Cas 22 57 41.2 +58 49 14.9 108.66 -0.86 12.9 3.3 D 13.6

Up: A catalogue of symbiotic