3. The list of candidates

The results of our search for new dwarf galaxy candidates are presented in Table 1 (click here) where Cols. 1, 2 are the equatorial coordinates (epoch 1950.0); Cols. 3, 4 are the major and minor angular diameters in arcmin measured on blue films; Col. 5 is the morphological type in usual designations ("d" as a "dwarf" was omitted); Col. 6 is the rough estimate of surface brightness (=SB): H -- high (equal or brighter than the SB of a normal spiral galaxy), L -- low, VL -- very low, EL -- extremely low (usually invisible on POSS-I but visible on POSS-II); Fig. 1 (click here) illustrates the appearence on the digital POSS-I of four objects with the different SB estimates; Col. 7 is the galaxy name or its number in the catalogues/lists : AM -- Arp & Madore (1987), FG -- Feitzinger & Galinski (1985), K -- Karachentseva (1968, 1972, 1973), BK -- Börngen & Karachentseva (1985), DDO -- van den Bergh (1966), UGC, UGCA (Nilson 1973, 1974), F -- Schombert et al. (1992), VCC -- Binggeli et al. (1985), MCG -- Vorontsov-Velyaminov et al. (1962-1968); Col. 8 contains the data on heliocentric radial velocities and galaxy shape and indicates some notes at the end of the Table 1 (click here). In preparing this article two HI surveys of nearby galaxies (Huchtmeier et al. 1997; Cote et al. 1997) revealed 15 our objects to have radial velocities greater than 1000 km/s. A list of them is presented in Table 2 (click here) where columns are the same as in Table 1 (click here).

The distribution of 260 galaxies from Table 1 (click here) is presented in Fig. 2 (click here) in equatorial coordinates. Because our survey does not cover the sky continuously, we do not discuss here the details of this distribution. Note only that the presented distribution delineates clearly the concentration toward the Local Supercluster plane and also the wide empty region coinciding with the Local Void (Tully 1988) around the direction , }.

  
Figure 1: Reproductions from the digital POSS-I of the objects: 0013-32 (SB = H), 1241+43 (SB = L), 1319-42 (SB = VL), and 1311+42 (SB = EL). Each chart is arcmin, North at top, East at left

  
Figure 2: Distribution of the Local Volume galaxy candidates in the equatorial coordinates

 

R.A. (1950.0) D. a b Type S.B. Identification Notes

1 2 3 4 5 6 7 8

00 12 31.6 -38 45 43 0.9 0.35 Im H AM 0012-384

00 12 53.5 -21 43 17 2.3 1.3 S0 H NGC 59 V=382 km/s [1]

00 13 00.0 -32 27 36 1.5 1.3 Ir/Sph H FG 11 granul.,undet.HI [2]

00 29 27.4 -33 32 30 0.9 0.8 Sph/Ir L FG 16,AM 0029-333

00 32 52.7 +36 13 21 5: 3: Sph EL And III

00 34 43.3 +47 53 57 0.5 0.45 Ir L distant?

00 35 18.6 -43 46 46 0.6 0.4 Im H AM 0035-434 undet.HI [2]

00 42 56.2 +37 45 51 4: 3: Sph EL And I

00 46 51.9 -18 20 48 1.2 1.1 Sph L K 2 dist.?undet.HI [2]

00 47 56.0 -20 10 44 1.3 1.2 Sph/Ir L FG 24 undet.HI [2]

01 06 03.4 -38 28 35 0.9 0.4 Im H K 3,AM 0106-382 distant?, V=645 [2]

01 13 41.9 +33 09 20 4: 2.5: Sph EL And II

01 39 29.5 +26 06 57 0.7 0.4 Ir L V= 359 [3]

01 41 54.0 +27 02 14 1.6 0.6 Ir L asym., V= 420 [3]

01 43 53.6 +26 33 07 0.6 0.2 Ir VL V= 368 [3]

01 52 30.2 +27 42 34 0.8 0.3 Ir L comp. N 784

01 57 18.1 +28 35 26 0.6 0.3 Ir L comp. N 784

01 57 22.0 +67 30 36 1.3 0.9 Sph? EL undet.HI [3]

02 02 02.4 +68 45 57 2.2 1.7 Ir L Cas 1 V= 35 [4]

02 31 39.9 +22 21 45 1.2 0.7 Sph VL

02 31 52.2 +59 09 42 2.4: 1.0: Ir EL MB 1 V= 189 [5]

02 51 54.1 +58 39 35 1.6 0.5 Ir EL

02 53 01.1 +58 42 37 2.0: 0.3: SB EL Cas 2 V= 112 [6]

02 53 54.5 +17 15 25 0.6 0.4 Ir? L distant?

03 07 59.9 +60 09 28 2.8 0.8 Ir? VL refl. neb.?

03 18 53.2 +62 36 27 1.8 0.9 Ir L undet.HI [3]

03 20 29.5 -66 30 04 1.2 0.4 Ir L EL in R

03 28 35.2 +47 37 28 1.4 0.8 Ir H UGC 2773 V= 231 [7]

03 33 18.9 -61 15 37 1.8 0.9 Im EL FG 82,AM 0333-611 resolved

03 37 12.6 +68 02 50 1.0 0.5 Sph? VL

03 37 26.2 -18 49 42 0.7 0.6 Ir/Sph L EL in R,dist.?

03 37 26.8 +19 35 30 0.8 0.7 Ir L undet.HI [3]

03 38 39.9 +67 52 57 0.4: 0.4: Ir VL

03 38 56.9 -45 30 52 1.5 1.5 Im H AM 0338-453 granulated

03 40 23.7 +67 42 26 2.5 1.7 Ir VL res?,undet.HI [3]

03 42 47.0 +67 30 57 1.0 0.6 Ir L distant?

03 47 15.0 +70 56 34 0.9 0.4 Ir? VL BK 17

03 58 47.0 -62 38 57 0.7 0.5 Im H AM 0358-623

04 00 06.0 +71 20 00 1.1: 0.9: Ir? EL refl.neb?,br.star

04 05 56.0 -55 27 21 1.6 1.0 Im H AM 0405-552 resolv?,pecul.

04 19 26.7 +72 41 27 3.7 2.1 Sph? VL Cam A comp. N 1560

04 39 44.4 +61 15 47 0.6 0.6 Ir? VL dist?,undet.HI [3]

04 45 11.0 -36 00 18 2.2 0.8 Im/Sm H AM 0445-360 resolved?

04 48 03.3 +67 01 02 2.2 1.1 Ir L V= 75 [3]

05 21 35.2 -34 37 13 0.55 0.4 Im H AM 0521-343 resolved?

05 23 05.4 -87 05 14 1.4 0.7 Im L FG154,AM0522-870 resolved?

05 27 49.0 -87 37 36 1.0 0.45 Im L AM 0528-873

05 28 26.3 -24 54 44 1.7: 0.3: Im/Sm VL AM 0528-245

05 39 00.7 +06 39 28 0.7 0.5 Im? H V= 441 [8]

05 47 25.5 +02 52 10 0.5 0.4 Ir VL shreded

05 48 47.9 +02 53 48 2.1 0.5 Ir EL obscured

06 02 18.4 -19 37 03 1.2 0.5 Ir L V= 645 [1]

06 12 51.5 -51 31 41 1.1 0.6 Im L AM 0612-513 resolved?

06 24 16.7 -26 14 06 0.6 0.3 Ir H AM 0624-261 V=495 [2],res.?

 

 

1 2 3 4 5 6 7 8

06 37 55.8 -40 40 24 0.7 0.45 Ir VL AM 0637-404 V=272+821 [9]

06 39 49.0 +36 41 03 1.3 0.4 Ir? L distant?

07 04 49.9 -21 57 29 1.9 1.1 Ir L V=+737 [1]

07 07 56.2 -51 23 08 1.4 1.1 Ir L FG 203

07 17 41.2 -57 19 06 2.1 1.6 Im/Sm VL FG 206,AM 0717-571 resolved?

07 20 23.0 +46 06 10 1.1 0.4 Ir L

07 29 13.1 +66 59 40 3: 2: Sph VL DDO 44 undet.HI [10],comp.N 2403

07 31 50.6 +42 12 13 0.6 0.4 Ir L

07 37 20.0 -69 13 38 1.5 0.9 Sph VL FG 219,AM 0737-691

07 39 30.0 +69 41 09 0.6 0.2 Ir L distant?

07 39 40.2 +16 40 47 0.9 0.5 Ir H comp. U 3974

07 44 05.4 +40 18 42 0.7 0.4 Ir L asymmetric

08 00 34.9 +15 17 03 1.0 0.5 Ir L

08 27 17.0 -84 58 57 1.1 1.0 Ir? H V=738 [1],pec.

08 49 44.1 +33 59 13 2.4: 1.8: Sph? EL comp.N 2683

08 52 16.3 +33 45 02 1.1 1.0 Sph? EL comp.N 2683

09 06 56.7 -23 09 51 0.45 0.35 Ir/Sph L AM 0906-231 dist?,undet.HI [9]

09 09 28.5 -23 46 35 0.6 0.5 Sph L EL in R

09 10 15.6 -24 02 05 0.9 0.8 Sph L EL in R,dist?

09 12 18.0 -23 20 55 0.8 0.4 Im L FG247,AM0912-232 dist?,undet.HI [9]

09 12 48.9 -25 40 30 0.9 0.6 Ir L VL in R

09 38 23.6 -76 21 41 2.1 0.8 Ir L refl.neb.?

09 46 08.5 +67 44 25 2.4 1.8 Sph VL comp. M 81

09 47 23.6 +31 41 26 0.5 0.3 Ir H UGC 5272B [11]

09 50 03.5 +29 32 46 0.6 0.4 BCD? H

09 50 45.0 +29 40 57 1.1 0.6 Ir L star projected

09 53 00.8 +68 49 47 2.6 2.6 Sph VL K 61 comp. M 81

10 00 25.3 -05 57 55 0.6 0.5 Ir L

10 01 18.0 +66 48 00 1.7 1.7 Sph VL DDO 71,K 63 comp. M 81

10 03 05.8 -07 30 20 1.9 1.3 Sph L K 65 comp. N 3115

10 03 09.0 +68 04 19 2.0 1.0 Sph L K 64,UGC 5442 comp. M 81

10 05 22.0 +30 44 09 1.0 0.6 Ir? L MCG 5-24-18 v.pecul., dist.?

10 12 37.6 -44 36 08 1.2 1.0 Sm? H AM 1012-443

10 13 57.4 -39 44 23 0.9 0.5 Ir VL AM 1013-394 V= 263+ 2982 [9]

10 22 47.6 +67 54 32 2.0 2.0 Sph VL DDO 78 comp. M 81

10 26 26.1 +23 01 57 1.0 0.15 Ir/S VL distant?

10 31 00.0 +66 16 00 1.0 0.8 Sph VL BK 6N comp. M 81

10 33 30.1 +27 47 52 0.8 0.7 Ir L

10 43 45.8 +14 17 16 1.2 1.1 Ir VL

10 44 18.1 +13 15 48 1.2 0.6 Ir VL near Leo tripl.

10 46 03.6 +64 59 20 2.2: 1.7: Ir VL UGCA 220

10 47 48.8 +12 37 34 1.2: 0.8: Sph EL near Leo tripl.

10 55 35.3 +20 22 35 0.7 0.5 Ir L near edge-on S

11 09 37.7 +17 01 32 0.9 0.4 Sph/Ir VL F 640-3 undet.HI [12]

11 11 11.2 -47 46 02 0.35 0.25 Im H AM 1111-474

11 11 22.9 +11 36 10 1.2 0.5 Ir VL distant ?

11 14 19.1 -32 22 39 0.7 0.4 Sph? L AM 1114-322 distant ?

11 20 21.2 +19 44 58 0.6 0.4 Ir? L F 570-3 undet.HI [12]

11 21 03.8 +19 31 52 0.6 0.4 Sph VL

11 26 14.5 +18 33 25 1.1 0.7 Ir? VL F 571-10 undet.HI [12]

11 26 40.7 +46 23 23 0.8 0.5 Ir? L

11 27 08.7 +52 40 54 0.8 0.7 Sph? VL K 78

11 31 40.1 +17 26 14 0.7 0.4 Ir L

11 37 23.0 +46 45 29 0.7 0.6 Sph? VL

 

1 2 3 4 5 6 7 8

11 44 33.5 +43 56 59 0.6 0.4 Ir? L

11 46 01.0 +56 11 44 0.6 0.6 Ir? L

11 51 27.3 +16 59 55 0.6 0.45 Ir? L Virgo member ?

11 52 10.5 -33 16 47 1.1 0.8 Ir L FG 315,AM 1152-331 V=640 [9]

11 52 17.9 +47 04 59 0.5 0.3 Ir? VL distant ?

11 53 55.1 -36 27 39 0.5 0.35 Im H

11 55 37.1 +49 09 34 0.7 0.55 Im H MCG 8-22-48

11 56 18.5 +46 00 45 1.3 0.7 Ir L UGCA 259 V=1154 [10],{*}

11 57 24.6 +44 59 50 0.6 0.6 Ir? L

11 58 42.9 +54 03 01 0.6 0.15 Ir VL

11 59 13.5 +28 38 26 0.8 0.7 Ir L distant ?

12 00 56.2 -25 11 35 2.5 1.9 Im/Sm L FG 320;AM 1200-251 filaments

12 02 52.3 +43 59 13 1.1 0.6 Ir VL

12 04 04.8 +55 02 38 1.0 0.25 Ir L

12 04 20.5 +17 37 01 0.9 0.2 Ir L Virgo member ?

12 06 16.1 +52 50 29 0.5 0.3 Ir? EL

12 10 16.9 +69 12 20 0.7 0.6 Sph? VL near br.star

12 10 47.5 +28 41 44 0.6 0.3 Ir L asymmetric

12 10 51.5 +30 12 00 0.9 0.25 Ir H V=152 [1],{*}

12 11 17.1 +05 37 54 0.6 0.4 Ir L GR 5

12 11 38.9 +16 14 35 1.1 1.1 Sph VL K 88,VCC 108 undet.HI [12]

12 15 17.6 +28 45 09 0.6 0.3 Ir L K 95

12 15 58.1 +28 55 31 0.6 0.5 Sph/Ir VL K 98

12 16 38.5 +48 00 25 0.6 0.5 Sph/Ir VL

12 17 04.1 +43 39 50 0.4 0.3 Ir L

12 17 05.3 +47 43 54 0.3 0.3 Sph? L

12 17 09.5 +58 19 18 0.8 0.4 Ir VL

12 18 13.5 +47 16 43 0.5 0.5 Sph? L

12 19 13.0 +38 15 06 0.9 0.5 Ir VL K 105

12 19 27.0 +28 31 09 0.9 0.5 Sph/Ir VL

12 19 37.9 +40 01 23 0.9 0.4 Ir L asym., dist.?

12 20 15.7 +08 11 27 0.6 0.5 Ir L VCC 584

12 20 23.2 +34 06 23 0.4 0.3 Ir L

12 21 48.5 -42 00 57 1.0 0.5 Ir? L AM 1221-420 star w.neb.?

12 22 34.0 +61 20 20 1.0 0.7 Ir L MCG 10-18-44

12 22 58.6 +28 45 33 1.5 0.5 Ir L

12 24 18.6 +62 39 23 1.1 0.7 Ir L UGC 7544 undet.HI [10]

12 24 19.1 +13 27 15 1.0 0.35 Sm L DDO 124 V=162 [10]

12 25 20.3 -37 03 12 2.0 0.25 Im/Sm? H AM 1225-370 resolved?

12 25 32.4 +22 51 57 0.8 0.4 Ir H UGC 7584

12 26 25.8 +42 27 20 0.8 0.45 Ir L MCG 7-26-11 V=408 [13]

12 27 28.2 +08 12 24 1.1 0.7 Im L UGC 7636 V=468 [10]

12 27 57.5 +43 10 38 1.2 0.5 Ir? L MCG 7-26-12 V=440 [13]

12 30 58.4 +33 37 42 1.2 0.4 Ir H MCG 06-28-9 granulated

12 32 44.4 +58 39 45 0.5 0.3 Ir L K 162 distant?

12 34 56.4 +39 01 12 0.7 0.4 Ir H Arp 211

12 35 13.0 +07 22 42 1.2 1.0 Ir L UGC 7795 V=61 [10]

12 38 09.0 +47 38 21 0.5 0.2 Ir L

12 38 31.3 -40 53 03 1.7 0.4 Ir VL AM 1238-405

12 39 06.9 +40 05 13 1.1 0.7 Ir L granulated

12 40 48.0 +35 41 16 0.7 0.5 Ir? L distant?

12 41 35.8 +43 56 15 0.8 0.6 Ir L

 

1 2 3 4 5 6 7 8

12 42 10.0 +71 03 52 1.1 0.7 Ir? L K 195

12 42 57.3 +18 34 25 0.9 0.7 Ir? EL {*}

12 43 37.6 +62 14 21 0.9 0.4 Ir? VL

12 45 26.9 +04 42 24 1.1 0.6 Ir H distant?

12 46 27.6 +32 14 33 0.7 0.7 Ir? L

12 46 49.5 +35 53 05 1.7 1.0 Sph L

12 49 17.8 +26 22 56 0.8 0.5 Ir? L distant?

12 50 37.8 +03 42 44 0.5 0.4 Ir? VL

12 50 41.3 +12 54 24 0.8 0.6 Ir L

12 52 11.5 -28 04 12 0.8 0.6 Im L AM 1252-280 V=645 [14]

12 53 03.1 +33 15 22 0.7 0.6 Ir? L distant?

12 54 14.0 +12 12 10 1.3 1.0 Ir L UGC 8061

12 56 07.5 +18 04 58 0.7 0.45 Ir L Virgo member?

12 56 29.7 -49 21 08 2.2 1.6 Ir L FG 363 V=1895 [10],{*}

12 56 38.7 +35 45 03 0.6 0.4 Ir? L

12 57 17.1 -19 08 26 1.7 0.7 Sph/Ir VL EL in R

13 00 15.2 +22 16 02 0.8 0.7 Sph? VL F 575-1 undet.HI [12]

13 00 32.8 +26 20 46 0.8 0.3 Ir L F 508-1

13 00 40.5 -46 19 07 1.2: 0.9: Sph L FG 367,AM 1300-461 comp. N 5128

13 02 02.1 +18 01 37 1.4 0.7 Sph/Ir VL F 575-4 undet.HI [12]

13 02 09.2 +27 02 31 0.7 0.6 Ir L

13 02 12.8 -39 48 54 1.0 0.55 Ir L fan-like, V= 619 [2]

13 04 14.8 +18 16 08 0.6 0.45 Sph? L

13 06 15.0 -50 44 46 1.9 0.4 Ir H AM 1305-501 distant?

13 06 36.8 +33 28 07 0.6 0.5 Ir L

13 07 03.5 -23 16 35 0.7 0.3 Im H AM 1307-231

13 07 23.3 -26 19 43 1.0 0.8 Im H AM 1307-263 granulated?

13 08 47.7 +37 26 39 0.9 0.6 Ir L

13 09 53.2 -41 34 01 1.0 0.6 Sph? VL EL in R, comp. N 5128

13 10 14.6 -44 37 28 2.7 1.7 Sph L FG 373,AM 1310-443 comp. N 5128

13 11 24.8 +42 18 31 0.8 0.7 Sph? EL comp. N 5055

13 12 02.7 +36 50 08 0.7 0.5 Sph? L

13 13 16.4 +41 45 55 0.6: 0.6: Ir/Sph EL

13 15 07.3 +44 39 44 0.6: 0.4: Ir? VL

13 18 20.5 -31 16 05 1.3 0.6 Ir VL EL in R

13 18 49.9 -44 48 05 0.6 0.4 Ir? L AM 1318-444

13 19 06.8 -42 16 20 1.5 1.1 Sph VL comp. N 5128

13 20 07.0 -33 18 23 0.6 0.5 Sph? L CEN 8

13 20 31.4 -28 56 34 0.4 0.35 Ir EL

13 21 48.1 -30 42 43 1.3 0.8 Im H K 15,AM 1321-304 V=490 [14]

13 22 20.0 -37 21 50 1.3 0.7 Ir/Sph VL AM 1321-372 near br.star

13 22 37.7 -29 00 39 0.6 0.45 Ir L

13 24 29.6 -45 05 36 0.5 0.5 Ir/Sph L AM 1324-450

13 25 28.7 -37 54 37 1.6 1.1 Ir? L FG 393,AM 1325-375

13 26 46.8 +67 53 28 1.2 0.5 Ir L UGC 8509 undet.HI [10]

13 31 18.6 +49 21 30 1.0 0.6 Ir H MCG 8-25-18

13 31 31.6 +56 45 26 0.6 0.4 Ir? VL

13 33 46.5 -29 19 00 6:: 2.5: Ir EL {*}

13 35 52.8 +49 22 26 0.4 0.25 Ir L

13 37 31.2 -31 26 47 1.4 0.6 Im? L FG 403 distant?

13 39 03.4 -44 57 11 1.2 1.1 Sph? L AM 1339-445 comp. N 5128

13 39 12.6 +43 32 31 0.8 0.6 Ir? L MCG 07-28-51 distant?

13 40 34.6 -43 31 04 0.6 0.3 Sph? VL EL in R

13 40 44.0 -45 29 41 0.75 0.4 Ir L AM 1340-453 distant?

 

1 2 3 4 5 6 7 8

13 40 45.2 -45 39 22 0.5 0.5 Im L AM 1340-453

13 41 24.2 +43 42 43 1.1 0.5 Ir H UGC 8688

13 43 13.4 -45 26 06 1.0 0.9 Sph L AM 1343-452 comp. N 5128

13 43 48.7 -29 43 47 1.7 0.7 Sph? VL comp. N 5236

13 45 21.9 +39 37 26 0.7 0.4 Ir? L

13 45 22.2 +33 27 25 0.8: 0.7: Ir L

13 45 40.5 -46 44 54 1.5: 1.0: Sph? EL near br.star

13 46 04.9 -47 57 21 0.5 0.4 Ir/Sph L AM 1346-475

13 46 07.8 +40 48 08 0.4 0.3 Ir? L granulated?

13 46 52.8 +43 50 54 1.0 0.4 Ir L distant?

13 52 51.5 +37 55 42 0.45 0.3 Ir L

13 53 01.2 -45 24 47 1.1 0.7 Ir L

13 54 03.7 +40 32 50 0.7 0.45 Ir L comp. N 5371?

13 57 21.1 +52 36 16 0.9 0.8 Ir? L UGC 8914 undet.HI [10], dist?

13 59 54.3 -46 51 45 0.8 0.6 Ir L AM 1359-465

14 05 01.5 +35 18 09 0.6 0.5 Ir VL

14 15 34.6 +23 18 21 0.8 0.3 Ir L arched

14 40 48.0 +50 01 40 0.9 0.5 Ir VL patchy

14 45 51.4 +53 02 31 1.1 0.7 Ir L MCG 9-24-40 br.star projected

14 57 13.6 -51 31 55 1.7 0.6 Ir VL FG 434

15 03 11.2 -39 42 36 0.8 0.6 Ir L FG 438 distant?

15 04 09.5 +56 03 24 0.9 0.7 Sph? VL

15 06 46.1 +56 27 03 0.7 0.5 Ir? L K 233

15 11 59.0 -22 56 23 0.8 0.6 Im L FG 458,AM 1511-225

15 25 33.2 -42 36 36 1.9 0.7 Ir L FG 444

16 22 23.0 -59 50 33 2.9 0.7 Sm? L

16 22 59.4 -60 20 53 1.6 1.0 Ir VL FG 447

17 54 26.1 +70 07 09 0.8 0.6 Sph? EL comp. N 6503?

18 18 05.0 -62 17 44 0.9 0.6 Ir L FG 458,AM 1818-622

19 09 20.3 -61 59 57 0.45 0.45 Sph? L AM 1909-615

19 16 17.0 +63 52 54 1.5 1.2 BCD H NGC 6789 V=-157[1],{*}

20 00 48.0 -31 49 24 1.2: 0.5: Ir VL FG 492

20 04 51.7 -61 12 30 0.9 0.6 Ir L AM 2004-611

20 22 46.0 -71 34 23 0.8 0.4 Ir L FG 499 distant?

20 25 58.8 -31 51 07 0.8 0.4 Ir L AM 2025-315 distant?

20 29 14.4 +60 16 22 1.8 0.8 Ir VL UGC 11583 V=129 [3]

20 29 31.9 +60 11 03 1.6 0.8 Ir? VL V=126 [3]

20 30 33.5 +60 38 34 0.9 0.9 Sph? VL V=132 [3]

20 33 30.7 -69 21 58 1.0 0.9 Ir L AM 2033-692

20 33 46.2 +60 55 12 1.5 0.9 Ir? EL undet.HI [3],{*}

21 54 21.4 -60 32 42 2.5 1.2 Ir L FG 532,AM 2154-603

22 09 04.6 -43 25 29 0.6 0.5 Im L AM 2209-432

22 19 25.2 -48 39 26 2.2 1.3 Ir L FG 545

22 37 56.3 -31 03 40 1.6 0.8 Ir? L K 20,FG 554,AM 2237-310

23 09 36.4 -44 03 01 4: 2.2: Sm? L FG 569

23 11 46.9 -43 52 39 4.5 1.8 Ir VL {*} [1] Huchra J. (1995) [2] Cote S. et al. (1997) [3] Huchtmeier W.K. et al. (1997) [4] Huchtmeier W.K. et al. (1995) [5] Huchtmeier W.K. & van Driel W. (1996)

 

1156+46. V=1154 km/s and W=350 km/s contradict to the galaxy morphology.

1210+30. In spite of V=152 km/s, the galaxy looks like distant.

1242+18. The object looks like an emulsion defect.

1256-49. V=1895 km/s conflicts with the galaxy morphology.

1333-29. Perhaps it is an outer part of M 83.

1916+63. Resolved into stars with the 6-m telescope.

2033+60. May be a reflecting nebula.

2311-43. The system discovered by R.Cannon; near NGC 7531 with V=1598 km/s; perhaps a case similar to the LSBD "0110+008" near NGC 428 (Smoker et al. 1996).

 

R.A. (1950.0) D. a b Type S.B. Identification Notes

1 2 3 4 5 6 7 8

00 38 30.5 -26 32 28 0.6 0.3 Ir VL SC 27 V= 2694 [2]

01 43 55.7 +14 26 33 1.0 0.7 Ir H UGC 1242 V= 7389 [3]

01 47 10.5 +28 40 03 0.7 0.5 Ir L V= 3841 [3]

02 01 46.3 +72 30 23 0.8 0.8 Ir L V= 2918 [3]

03 29 09.1 +67 56 36 2.0 0.8 Ir L K 37=BK 7 V= 1372 [3]

03 33 44.4 +67 26 00 2.0 0.7 Ir? L BK 8 V= 1434 [3]

03 38 25.0 +68 06 11 2.2 0.3 Ir? L BK 12 V= 1320 [3]

03 53 22.5 +69 08 24 1.1 0.6 Sph? L BK 19 V= 1302 [3]

03 59 34.8 +71 25 44 1.2 0.5 Ir VL BK 21 V= 1734 [3]

04 06 44.0 +70 38 33 0.9 0.4 Ir L V= 1159 [3]

04 46 40.8 +67 04 29 0.6 0.4 Sph? L V= 1581 [3]

13 03 33.1 -49 33 38 1.6 0.6 Ir L V= 1281 [2]

13 41 52.9 -29 48 19 0.7 0.7 Im H FG 405,AM 1341-294 V= 4620 [2]

14 06 37.4 -30 02 30 0.8 0.6 Im H V= 2629 [2]

14 16 00.0 -45 05 15 1.2 0.6 Im H AM 1415-450 V= 1653 [2]