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Up: Search for young stars cloud


   
2 X-ray data reduction

The previously known young stars associated with the CrA dark cloud are located in a small, $\sim 126~{\rm deg} ^{2}$ area around R CrA near $\alpha _{2000} = 19^{\rm h}$ and $\delta _{2000} = -37 ^{\circ}$. Because we also expect to find previously unknown young stars around the dark cloud, we investigated the area $\alpha _{2000} = 18^{\rm h}~35^{\rm m}$ to $19^{\rm h}~38^{\rm m}$ and $\delta _{2000} = -41^{\circ}$ to $-33^{\circ}$.

We reduced all RASS II data[*] pertaining to that area with the Extended Scientific Analysis Software (EXSAS, Zimmermann et al. 1994) version 98APR running under ESO-MIDAS version 97NOV. We performed standard local and map source detection in the bands soft (0.1 to $0.4~{\rm keV}$), hard 1 (0.5 to $0.9~{\rm keV}$), hard 2 (0.9 to $2.0~{\rm keV}$), hard (0.5 to $2.0~{\rm keV}$), and broad (0.1 to $2.4~{\rm keV}$), as described in detail in Neuhäuser et al. (1995). After merging the source lists, each source was again tested in the above mentioned five bands by a maximum likelihood source detection algorithm. Following Neuhäuser et al. (1995) we accept only sources with $ML \ge 7.4$ corresponding to $\sim 3.5~\sigma$ as real.


   
Table 2: X-ray data for our sample. Listed are all X-ray sources detected in the ROSAT All-Sky Survey sorted by right ascension. We list a running number (used in other tables for cross-reference), the ROSAT source designation, the X-ray source position (J2000.0), the maximum likelihood of existence ML, the hardness ratios with errors, the (background subtracted and vignetting corrected) number of counts in the broad band (0.1 to $2.4~{\rm keV}$) with errors, the exposure time in seconds, and $\log ECF$ for the energy conversion factor in counts ${\rm erg^{-1}~cm^{2}}$
No. Designation $\alpha _{2000}$ (X-ray) $\delta _{2000}$ ML HR 1 HR 2 Counts Exp. [s] $\log ECF$
1 RXJ1835.1-3404 18:35:08.0 -34:04:20.0 10.2 $ \ge 0.61$ $ 0.30 \pm 0.36$ 8.9$~\pm~$ 4.0 147.2 -10.87
2 RXJ1835.3-3927 18:35:21.5 -39:27:13.3 8.1 $ 0.15 \pm 0.49$ $ \ge 0.10$ 7.1$~\pm~$ 3.2 124.3 -11.04
3 RXJ1835.7-3259 18:35:47.0 -32:59:41.5 1240.1 $ 0.93 \pm 0.02$ $ 0.53 \pm 0.05$ 364.0$~\pm~$19.6 163.0 -10.88
4 RXJ1835.8-3813 18:35:49.2 -38:13:24.1 9.8 $ 0.77 \pm 0.41$ $ 0.02 \pm 0.44$ 11.7$~\pm~$ 4.3 139.4 -10.91
5 RXJ1835.8-4046 18:35:53.4 -40:46:23.5 10.2 $ \ge 0.27$ $ \ge 0.43$ 3.6$~\pm~$ 2.3 125.7 -10.87
6 RXJ1835.9-3525 18:35:58.3 -35:25:35.5 7.7 $ 0.77 \pm 0.44$ $ \ge 0.42$ 6.1$~\pm~$ 3.4 143.3 -10.91
7 RXJ1836.3-4010 18:36:18.7 -40:10:20.2 13.1 $-0.65 \pm 0.40$ $ \le 0.19$ 11.2$~\pm~$ 4.0 131.5 -11.31
8 RXJ1836.6-3451 18:36:40.6 -34:51:33.5 13.2 $ \ge 0.44$ $ 0.28 \pm 0.42$ 9.4$~\pm~$ 3.9 139.1 -10.87
9 RXJ1837.3-3442 18:37:18.2 -34:42:39.0 13.1 $ 0.25 \pm 0.40$ $ 0.05 \pm 0.54$ 9.2$~\pm~$ 3.5 133.2 -11.02
10 RXJ1838.2-3838 18:38:17.1 -38:38:12.9 11.8 $ \ge 0.47$ $ 0.31 \pm 0.41$ 8.0$~\pm~$ 3.3 142.1 -10.87
11 RXJ1838.3-3523 18:38:20.2 -35:23:32.6 10.3 $-0.67 \pm 0.52$ $ \le 0.42$ 9.4$~\pm~$ 3.8 140.0 -11.32
12 RXJ1839.0-3705 18:39:05.8 -37:05:46.8 21.6 $ 0.84 \pm 0.24$ $-0.03 \pm 0.31$ 13.4$~\pm~$ 4.2 139.0 -10.89
13 RXJ1839.0-3726 18:39:05.9 -37:26:36.0 12.3 $ 0.78 \pm 0.21$ $-0.30 \pm 0.39$ 9.7$~\pm~$ 3.9 142.1 -10.90
14 RXJ1839.2-3854 18:39:16.1 -38:54:13.8 9.2 $ \ge 0.18$ $ \ge 0.40$ 3.3$~\pm~$ 2.5 135.4 -10.87
15 RXJ1839.7-3458 18:39:46.8 -34:58:58.2 7.8 $ \ge 0.55$ $ 0.51 \pm 0.35$ 5.8$~\pm~$ 3.2 167.4 -10.87
16 RXJ1840.1-3640 18:40:09.5 -36:40:09.1 7.9 $ 0.24 \pm 0.40$ $ 0.08 \pm 0.52$ 8.6$~\pm~$ 3.6 154.6 -11.02
17 RXJ1840.6-3728 18:40:38.3 -37:28:44.3 13.0 $ \ge 0.67$ $ 0.29 \pm 0.36$ 8.6$~\pm~$ 3.6 150.6 -10.87
18 RXJ1840.6-3612 18:40:39.7 -36:12:14.1 7.8 $ 0.34 \pm 0.37$ $-0.01 \pm 0.48$ 11.1$~\pm~$ 4.2 150.4 -10.99
19 RXJ1840.8-3547 18:40:53.8 -35:47:06.2 32.7 $-0.13 \pm 0.25$ $-0.19 \pm 0.38$ 20.2$~\pm~$ 5.0 147.3 -11.12
20 RXJ1840.9-3350 18:40:55.1 -33:50:52.5 14.9 $ 0.28 \pm 0.30$ $ 0.38 \pm 0.33$ 16.4$~\pm~$ 5.1 180.2 -11.01
21 RXJ1841.2-3821 18:41:13.5 -38:21:55.9 9.1 $ \le -0.49$   5.7$~\pm~$ 3.1 151.9 -11.52
22 RXJ1841.5-3508 18:41:34.2 -35:08:27.7 11.2 $ 0.15 \pm 0.38$ $-0.28 \pm 0.53$ 9.5$~\pm~$ 3.8 154.7 -11.04
23 RXJ1841.8-3525 18:41:49.7 -35:25:44.3 58.2 $ 0.47 \pm 0.18$ $-0.14 \pm 0.24$ 26.6$~\pm~$ 5.6 140.0 -10.97
24 RXJ1842.1-3732 18:42:12.0 -37:32:33.0 9.4 $ 0.05 \pm 0.38$ $-0.09 \pm 0.53$ 9.7$~\pm~$ 3.8 141.1 -11.07
25 RXJ1842.8-3845 18:42:48.6 -38:45:28.3 8.7 $ \ge 0.40$ $ 0.46 \pm 0.45$ 8.7$~\pm~$ 3.6 137.4 -10.87
26 RXJ1842.9-3451 18:42:58.2 -34:51:00.3 7.6 $ 0.95 \pm 0.50$ $ \ge 0.22$ 3.7$~\pm~$ 2.4 154.3 -10.87
27 RXJ1842.9-3532 18:42:58.4 -35:32:34.6 21.7 $ 0.90 \pm 0.24$ $ 0.29 \pm 0.34$ 10.9$~\pm~$ 3.9 135.3 -10.88
28 RXJ1843.0-3331 18:43:05.2 -33:31:07.6 8.1 $ 0.35 \pm 0.40$ $ 0.14 \pm 0.49$ 8.7$~\pm~$ 3.9 191.5 -10.99
29 RXJ1843.4-3314 18:43:24.5 -33:14:31.4 11.8 $-0.51 \pm 0.35$ $ \le 0.32$ 14.3$~\pm~$ 5.0 194.2 -11.25
30 RXJ1844.3-3541 18:44:19.5 -35:41:43.5 30.0 $ 0.70 \pm 0.19$ $ 0.12 \pm 0.26$ 24.5$~\pm~$ 5.8 149.5 -10.92
31 RXJ1844.5-3723 18:44:31.1 -37:23:59.8 43.4 $ 0.62 \pm 0.20$ $ 0.18 \pm 0.26$ 23.2$~\pm~$ 5.2 141.1 -10.94
32 RXJ1844.5-3739 18:44:31.3 -37:39:13.9 10.4 $ 0.53 \pm 0.46$ $ \ge 0.24$ 6.9$~\pm~$ 3.3 134.9 -10.95
33 RXJ1844.7-3313 18:44:43.4 -33:13:56.1 8.9 $ 0.83 \pm 0.31$ $ 0.78 \pm 0.47$ 7.4$~\pm~$ 3.8 206.1 -10.90
34 RXJ1844.7-3450 18:44:45.9 -34:50:55.2 7.9 $ 0.68 \pm 0.65$ $ \ge 0.41$ 4.8$~\pm~$ 2.9 185.1 -10.92
35 RXJ1845.1-3324 18:45:10.4 -33:24:26.3 10.6 $-0.28 \pm 0.38$ $ 0.20 \pm 0.62$ 9.6$~\pm~$ 3.9 200.1 -11.16
36 RXJ1845.5-3750 18:45:34.4 -37:50:24.3 57.7 $ 0.59 \pm 0.15$ $ 0.28 \pm 0.18$ 39.6$~\pm~$ 6.9 143.7 -10.94
37 RXJ1846.3-3552 18:46:18.9 -35:52:34.0 7.9 $ \le -0.34$   5.6$~\pm~$3.0 161.1 -11.52
38 RXJ1846.7-3604 18:46:44.3 -36:04:40.4 8.0 $ \ge -0.09$ $ 0.06 \pm 0.59$ 5.1$~\pm~$ 2.9 143.7 -10.87
39 RXJ1846.7-3636 18:46:46.2 -36:36:21.3 29.2 $ 0.07 \pm 0.27$ $ 0.20 \pm 0.36$ 19.1$~\pm~$ 4.9 142.0 -11.06
40 RXJ1846.8-3911 18:46:53.3 -39:11:10.3 7.8 $ 0.45 \pm 0.42$ $-0.12 \pm 0.49$ 8.9$~\pm~$ 3.6 125.3 -10.97
41 RXJ1846.9-3503 18:46:58.0 -35:03:59.4 9.1 $ 0.84 \pm 0.33$ $ \le -0.59$ 7.9$~\pm~$ 3.8 176.3 -10.89
42 RXJ1847.2-3709 18:47:14.3 -37:09:43.3 8.6 $ 0.47 \pm 0.42$ $ \le -0.30$ 6.5$~\pm~$ 3.2 136.3 -10.97
43 RXJ1847.5-3642 18:47:32.9 -36:42:43.9 9.6 $ 0.93 \pm 0.44$ $ 0.13 \pm 0.52$ 4.6$~\pm~$ 2.3 136.0 -10.88
44 RXJ1847.7-3606 18:47:46.5 -36:06:12.4 29.7 $ \ge 0.68$ $ 0.14 \pm 0.28$ 15.7$~\pm~$ 4.4 154.3 -10.87
45 RXJ1847.7-4024 18:47:46.9 -40:24:14.2 69.8 $ 0.00 \pm 0.19$ $ 0.35 \pm 0.24$ 36.7$~\pm~$ 6.5 130.2 -11.08
46 RXJ1847.8-3828 18:47:51.9 -38:28:45.9 7.4 $ \ge 0.19$ $ \ge 0.23$ 2.2$~\pm~$ 1.7 122.5 -10.87
47 RXJ1848.2-3415 18:48:12.1 -34:15:41.3 8.2 $ 0.42 \pm 0.39$ $-0.16 \pm 0.47$ 9.4$~\pm~$ 4.0 202.0 -10.98
48 RXJ1848.6-3458 18:48:36.1 -34:58:58.0 8.0 $ 0.08 \pm 0.59$ $ 0.22 \pm 0.85$ 8.7$~\pm~$ 3.8 200.2 -11.06
49 RXJ1849.0-3734 18:49:02.0 -37:34:22.7 9.6 $ \ge 0.40$ $-0.44 \pm 0.41$ 6.0$~\pm~$ 3.0 157.8 -10.87
50 RXJ1849.1-3546 18:49:08.7 -35:46:41.7 45.0 $ 0.71 \pm 0.17$ $ 0.56 \pm 0.20$ 22.5$~\pm~$ 5.2 193.1 -10.92
51 RXJ1851.4-3455 18:51:26.1 -34:55:31.6 8.1 $ \ge 0.39$ $-0.45 \pm 0.48$ 5.3$~\pm~$ 3.0 211.0 -10.87
52 RXJ1852.1-3607 18:52:10.2 -36:07:24.9 7.8 $ 0.19 \pm 0.39$ $-0.57 \pm 0.43$ 9.4$~\pm~$ 3.8 171.9 -11.03


Table 2. continued
No. Designation $\alpha _{2000}$ (X-ray) $\delta _{2000}$ ML HR 1 HR 2 Counts Exp. [s] $\log ECF$
53 RXJ1852.3-3700 18:52:18.2 -37:00:20.4 36.3 $ 0.90 \pm 0.13$ $ 0.54 \pm 0.25$ 14.7$~\pm~$ 4.3 155.5 -10.88
54 RXJ1852.4-3730 18:52:25.6 -37:30:32.4 54.4 $-0.41 \pm 0.19$ $-0.26 \pm 0.38$ 29.4$~\pm~$ 6.0 152.8 -11.21
55 RXJ1853.1-3609 18:53:06.5 -36:09:54.7 55.5 $ 0.33 \pm 0.18$ $ 0.40 \pm 0.22$ 37.1$~\pm~$ 6.8 190.8 -11.00
56 RXJ1853.4-4020 18:53:26.3 -40:20:02.8 9.2 $-0.18 \pm 0.49$ $ \le 0.01$ 7.7$~\pm~$ 3.4 147.6 -11.13
57 RXJ1853.5-3544 18:53:36.0 -35:44:32.7 9.4 $ \ge 0.34$ $ 0.10 \pm 0.48$ 6.4$~\pm~$ 3.3 214.1 -10.87
58 RXJ1854.4-4010 18:54:25.7 -40:10:21.7 9.3 $ \ge 0.32$ $ 0.40 \pm 0.48$ 7.1$~\pm~$ 3.4 154.8 -10.87
59 RXJ1854.4-3738 18:54:28.2 -37:38:39.7 7.7 $ \ge 0.37$ $ 0.39 \pm 0.44$ 6.0$~\pm~$ 3.1 173.8 -10.87
60 RXJ1854.5-3823 18:54:34.3 -38:23:22.2 8.5 $-0.31 \pm 0.42$ $ \le -0.27$ 13.0$~\pm~$ 4.6 161.7 -11.18
61 RXJ1854.9-3600 18:54:59.4 -36:00:26.0 8.9 $ \ge 0.40$ $-0.47 \pm 0.44$ 9.5$~\pm~$ 4.0 232.8 -10.87
62 RXJ1855.5-3806 18:55:32.5 -38:06:41.2 12.7 $ \ge 0.58$ $ 0.76 \pm 0.32$ 8.4$~\pm~$ 4.0 171.9 -10.87
63 RXJ1856.5-3754 18:56:35.1 -37:54:32.7 2643.8 $-0.92 \pm 0.02$ $-0.94 \pm 0.16$ 637.3$~\pm~$25.5 166.8 -11.46
64 RXJ1856.6-3545 18:56:43.7 -35:45:23.1 8.9 $ \ge 0.07$ $ 0.22 \pm 0.28$ 4.7$~\pm~$ 2.7 216.0 -10.87
65 RXJ1856.7-4021 18:56:46.2 -40:21:10.7 12.0 $ \ge 0.52$ $ 0.61 \pm 0.37$ 7.0$~\pm~$ 3.5 166.0 -10.87
66 RXJ1857.3-3635 18:57:19.8 -36:35:49.3 10.6 $-0.45 \pm 0.38$ $-0.78 \pm 1.33$ 11.4$~\pm~$ 4.2 211.7 -11.23
67 RXJ1857.3-3554 18:57:22.4 -35:54:19.4 10.0 $ \le -0.45$ $ \ge -0.65$ 6.7$~\pm~$ 3.3 244.5 -11.52
68 RXJ1857.5-3732 18:57:33.7 -37:32:57.3 10.5 $ 0.78 \pm 0.37$ $ 0.95 \pm 0.37$ 5.8$~\pm~$ 2.9 176.8 -10.90
69 RXJ1857.9-3651 18:58:00.1 -36:51:10.7 8.5 $ \le -0.43$ $ \ge -0.83$ 8.3$~\pm~$ 3.8 225.4 -11.52
70 RXJ1858.0-3640 18:58:05.3 -36:40:57.2 8.1 $-0.01 \pm 0.41$ $-0.44 \pm 0.47$ 10.3$~\pm~$ 4.3 236.1 -11.08
71 RXJ1858.4-3446 18:58:29.4 -34:46:53.2 32.1 $ 0.83 \pm 0.16$ $-0.32 \pm 0.23$ 27.8$~\pm~$ 6.4 312.3 -10.90
72 RXJ1858.6-3630 18:58:40.4 -36:30:38.8 12.3 $-0.17 \pm 0.35$ $ 0.42 \pm 0.45$ 12.5$~\pm~$ 4.6 257.0 -11.13
73 RXJ1858.7-3706 18:58:43.5 -37:06:18.3 25.1 $-0.19 \pm 0.27$ $ 0.22 \pm 0.49$ 20.9$~\pm~$ 5.3 229.4 -11.14
74 RXJ1859.0-4051 18:59:01.1 -40:51:19.5 8.5 $ \ge 0.14$ $ \le -0.23$ 6.0$~\pm~$ 3.2 154.6 -10.87
75 RXJ1859.3-3406 18:59:21.7 -34:06:09.9 7.5 $ \ge 0.55$ $-0.16 \pm 0.42$ 6.1$~\pm~$ 3.7 300.1 -10.87
76 RXJ1900.6-3810 19:00:38.9 -38:10:19.5 14.2 $ 0.99 \pm 0.15$ $ 0.27 \pm 0.30$ 13.4$~\pm~$ 4.9 234.9 -10.87
77 RXJ1900.8-3453 19:00:51.4 -34:53:08.0 7.9 $ 0.99 \pm 0.44$ $ 0.10 \pm 0.39$ 9.9$~\pm~$ 4.3 296.8 -10.87
78 RXJ1900.9-3928 19:00:59.6 -39:28:55.6 10.3 $ \ge 0.54$ $-0.43 \pm 0.35$ 8.1$~\pm~$ 3.8 190.4 -10.87
79 RXJ1901.1-3333 19:01:08.8 -33:33:40.8 8.9 $ \ge 0.39$ $ \le -0.35$ 3.6$~\pm~$ 2.4 233.9 -10.87
80 RXJ1901.1-3648 19:01:09.2 -36:48:01.7 9.8 $ 0.42 \pm 0.39$ $ 0.44 \pm 0.42$ 9.7$~\pm~$ 4.0 272.1 -10.98
81 RXJ1901.4-4022 19:01:24.6 -40:22:31.9 11.3 $ 0.63 \pm 0.63$ $-0.17 \pm 0.46$ 11.0$~\pm~$ 4.2 188.3 -10.93
82 RXJ1901.4-3422 19:01:26.8 -34:22:44.8 48.4 $ 0.11 \pm 0.19$ $-0.40 \pm 0.23$ 37.7$~\pm~$ 7.1 295.0 -11.05
83 RXJ1901.5-3700 19:01:31.4 -37:00:55.1 37.7 $ 0.83 \pm 0.17$ $-0.06 \pm 0.22$ 26.8$~\pm~$ 6.1 268.0 -10.90
84 RXJ1901.6-3652 19:01:38.9 -36:52:55.0 38.3 $ 0.80 \pm 0.18$ $ 0.54 \pm 0.20$ 24.6$~\pm~$ 5.8 278.8 -10.90
85 RXJ1901.6-3644 19:01:39.0 -36:44:52.4 27.1 $ \ge 0.61$ $ 0.95 \pm 0.15$ 15.2$~\pm~$ 4.8 279.1 -10.87
86 RXJ1902.0-3822 19:02:03.1 -38:22:02.4 8.9 $ 0.15 \pm 0.42$ $ \ge 0.21$ 8.3$~\pm~$ 3.5 237.5 -11.04
87 RXJ1902.0-3707 19:02:03.1 -37:07:47.7 22.6 $ 0.71 \pm 0.21$ $ 0.58 \pm 0.24$ 17.5$~\pm~$ 4.8 268.1 -10.92
88 RXJ1902.3-3310 19:02:20.0 -33:10:45.8 8.0 $-0.82 \pm 0.47$   8.1$~\pm~$ 3.7 187.4 -11.40
89 RXJ1902.3-3655 19:02:22.7 -36:55:42.8 7.5 $ \ge 0.07$ $ 0.76 \pm 0.38$ 4.8$~\pm~$ 2.8 282.5 -10.87
90 RXJ1902.3-3922 19:02:22.8 -39:22:11.2 9.5 $-0.32 \pm 0.44$ $-0.64 \pm 0.85$ 9.4$~\pm~$ 3.8 204.3 -11.18
91 RXJ1902.4-3617 19:02:24.0 -36:17:53.5 7.6 $ \ge 0.54$ $-0.06 \pm 0.48$ 4.1$~\pm~$ 2.7 306.9 -10.87
92 RXJ1902.5-3504 19:02:31.6 -35:04:58.8 9.5 $ \le -0.58$   7.0$~\pm~$ 3.6 305.2 -11.52
93 RXJ1902.7-3418 19:02:45.6 -34:18:36.0 8.8 $ \ge 0.47$ $ 0.67 \pm 0.46$ 5.3$~\pm~$ 3.3 288.8 -10.87
94 RXJ1903.0-3906 19:03:01.6 -39:06:09.4 12.9 $ \ge 0.50$ $ 0.20 \pm 0.37$ 10.4$~\pm~$ 4.1 222.5 -10.87
95 RXJ1903.0-4009 19:03:03.4 -40:09:09.7 18.6 $ 0.63 \pm 0.34$ $ 0.03 \pm 0.34$ 13.6$~\pm~$ 4.3 194.3 -10.93
96 RXJ1904.0-3817 19:04:01.7 -38:17:05.0 7.7 $ \ge 0.28$ $ \le -0.39$ 4.4$~\pm~$ 2.8 286.9 -10.87
97 RXJ1904.0-3804 19:04:04.0 -38:04:19.0 10.2 $-0.64 \pm 0.39$ $-0.76 \pm 1.61$ 13.5$~\pm~$ 4.8 299.3 -11.31
98 RXJ1904.0-3824 19:04:04.7 -38:24:56.8 7.4 $ \le -0.14$   5.2$~\pm~$ 3.0 293.0 -11.52
99 RXJ1904.3-3835 19:04:23.7 -38:35:15.9 10.6 $ \ge 0.42$ $ \ge 0.36$ 7.4$~\pm~$ 3.8 289.8 -10.87
100 RXJ1904.5-3307 19:04:34.0 -33:07:16.0 8.0 $ 0.91 \pm 0.38$ $ 0.27 \pm 0.39$ 7.9$~\pm~$ 3.7 115.6 -10.88
101 RXJ1904.5-4028 19:04:34.4 -40:28:31.9 7.5 $ \le -0.29$ $ \le 0.77$ 7.4$~\pm~$ 3.8 218.5 -11.52
102 RXJ1904.6-4048 19:04:36.4 -40:48:24.2 8.9 $ \ge 0.42$ $-0.15 \pm 0.44$ 7.3$~\pm~$ 3.4 211.3 -10.87
103 RXJ1904.7-3604 19:04:43.8 -36:04:58.5 17.8 $ 0.60 \pm 0.26$ $ 0.33 \pm 0.29$ 17.6$~\pm~$ 5.1 326.7 -10.94
104 RXJ1905.0-3817 19:05:04.9 -38:17:46.3 9.6 $ 0.09 \pm 0.36$ $-0.04 \pm 0.49$ 11.7$~\pm~$ 4.3 313.2 -11.06
105 RXJ1905.0-3629 19:05:05.2 -36:29:14.0 8.8 $ 0.86 \pm 0.74$ $ \le -0.50$ 6.8$~\pm~$ 3.6 332.1 -10.89
106 RXJ1905.3-3855 19:05:18.8 -38:55:15.1 12.1 $ 0.70 \pm 0.33$ $ 0.07 \pm 0.35$ 17.5$~\pm~$ 5.1 304.2 -10.92
107 RXJ1905.3-4030 19:05:19.6 -40:30:59.1 8.5 $-0.34 \pm 0.36$ $-0.28 \pm 0.71$ 12.3$~\pm~$ 4.5 247.9 -11.19
108 RXJ1906.4-3703 19:06:25.0 -37:03:34.9 25.2 $-0.80 \pm 0.25$ $ \ge -0.10$ 14.3$~\pm~$ 4.2 325.1 -11.39
109 RXJ1906.5-3932 19:06:31.9 -39:32:58.1 8.8 $-0.93 \pm 0.55$ $ \le 0.06$ 8.6$~\pm~$ 3.9 289.6 -11.47


Table 2. continued
No. Designation $\alpha _{2000}$ (X-ray) $\delta _{2000}$ ML HR 1 HR 2 Counts Exp. [s] $\log ECF$
110 RXJ1906.8-3748 19:06:51.2 -37:48:40.3 12.8 $ \le -0.55$   8.4$~\pm~$ 3.4 325.3 -11.52
111 RXJ1907.8-3923 19:07:50.8 -39:23:39.8 74.9 $ \ge 0.82$ $ 0.33 \pm 0.18$ 28.8$~\pm~$ 5.9 294.9 -10.87
112 RXJ1909.6-3949 19:09:40.9 -39:49:37.6 35.1 $ 0.52 \pm 0.22$ $ 0.26 \pm 0.26$ 20.4$~\pm~$ 5.0 322.2 -10.96
113 RXJ1909.8-3343 19:09:50.9 -33:43:17.9 10.6 $ \le -0.31$   7.0$~\pm~$ 3.4 222.6 -11.52
114 RXJ1910.8-3854 19:10:48.8 -38:54:48.4 20.0 $-0.04 \pm 0.27$ $-0.42 \pm 0.36$ 20.7$~\pm~$ 5.4 351.6 -11.09
115 RXJ1911.5-3434 19:11:34.8 -34:34:59.3 40.6 $ 0.68 \pm 0.17$ $ 0.13 \pm 0.24$ 26.9$~\pm~$ 6.0 323.7 -10.92
116 RXJ1911.7-3641 19:11:47.4 -36:41:54.9 11.3 $-0.76 \pm 0.41$ $ 0.81 \pm 1.14$ 10.3$~\pm~$ 3.9 320.2 -11.37
117 RXJ1912.6-3431 19:12:36.6 -34:31:40.5 16.7 $ 0.57 \pm 0.34$ $ 0.09 \pm 0.36$ 13.8$~\pm~$ 4.5 322.2 -10.95
118 RXJ1913.0-3633 19:13:01.2 -36:33:04.4 22.2 $ 0.68 \pm 0.24$ $ 0.00 \pm 0.30$ 16.4$~\pm~$ 4.7 319.0 -10.92
119 RXJ1913.1-3622 19:13:10.2 -36:22:06.1 8.6 $ \ge 0.39$ $-0.59 \pm 0.38$ 7.6$~\pm~$ 3.5 318.8 -10.87
120 RXJ1913.3-3530 19:13:21.8 -35:30:40.1 8.3 $ \ge 0.27$ $ \le -0.35$ 4.7$~\pm~$ 2.8 317.9 -10.87
121 RXJ1913.6-3543 19:13:36.6 -35:43:10.1 11.7 $ \ge 0.54$ $ \le -0.39$ 5.8$~\pm~$ 3.3 307.7 -10.87
122 RXJ1913.7-3303 19:13:46.3 -33:03:59.8 9.3 $ 0.51 \pm 0.32$ $-0.15 \pm 0.42$ 10.8$~\pm~$ 4.1 194.9 -10.96
123 RXJ1913.8-3347 19:13:50.2 -33:47:49.1 13.9 $-0.06 \pm 0.38$ $ 0.36 \pm 0.55$ 15.8$~\pm~$ 5.2 275.4 -11.10
124 RXJ1914.4-3532 19:14:28.9 -35:32:27.2 8.1 $ \ge 0.14$ $ \le -0.19$ 7.5$~\pm~$ 3.6 292.3 -10.87
125 RXJ1914.6-3601 19:14:36.3 -36:01:12.9 8.0 $ \le -0.37$   8.4$~\pm~$ 4.0 286.1 -11.52
126 RXJ1915.5-3759 19:15:32.2 -37:59:35.3 8.5 $ \le -0.49$   4.6$~\pm~$ 2.7 316.6 -11.52
127 RXJ1915.5-3528 19:15:34.3 -35:28:45.2 7.8 $ 0.69 \pm 0.43$ $-0.42 \pm 0.36$ 9.8$~\pm~$ 4.2 283.4 -10.92
128 RXJ1915.7-3321 19:15:46.7 -33:21:58.7 9.7 $ \ge 0.37$ $-0.59 \pm 0.37$ 5.7$~\pm~$ 2.9 228.0 -10.87
129 RXJ1915.9-3350 19:15:58.7 -33:50:47.7 9.3 $ \ge 0.31$ $ \le -0.50$ 5.1$~\pm~$ 3.2 267.5 -10.87
130 RXJ1916.2-3548 19:16:13.1 -35:48:20.1 11.3 $ 0.57 \pm 0.25$ $-0.35 \pm 0.37$ 13.6$~\pm~$ 4.6 283.9 -10.94
131 RXJ1916.5-3458 19:16:33.7 -34:58:55.7 9.2 $ \le -0.35$ $ \le 0.47$ 9.2$~\pm~$ 4.1 292.7 -11.52
132 RXJ1916.9-4024 19:16:58.2 -40:24:32.0 7.8 $-0.85 \pm 0.45$ $ \ge -0.50$ 6.0$~\pm~$ 2.9 246.5 -11.42
133 RXJ1917.0-3331 19:17:04.0 -33:31:04.4 28.0 $ \ge 0.63$ $ 0.77 \pm 0.19$ 17.0$~\pm~$ 5.0 219.5 -10.87
134 RXJ1917.2-3931 19:17:12.9 -39:31:25.8 7.6 $ \ge 0.20$ $ \le -0.06$ 4.1$~\pm~$ 2.5 287.9 -10.87
135 RXJ1917.4-3756 19:17:24.3 -37:56:55.4 122.6 $ 0.46 \pm 0.12$ $ 0.08 \pm 0.16$ 58.1$~\pm~$ 8.2 310.7 -10.97
136 RXJ1917.8-3927 19:17:51.3 -39:27:33.4 7.8 $ \ge 0.41$ $-0.16 \pm 0.47$ 5.7$~\pm~$ 3.1 286.2 -10.87
137 RXJ1918.0-4000 19:18:00.7 -40:00:28.6 7.6 $ 0.25 \pm 0.46$ $ \ge 0.24$ 6.7$~\pm~$ 3.2 250.7 -11.02
138 RXJ1918.2-3823 19:18:12.9 -38:23:05.8 1044.6 $-0.08 \pm 0.06$ $ 0.20 \pm 0.08$ 319.8$~\pm~$18.3 307.7 -11.10
139 RXJ1918.4-3913 19:18:25.1 -39:13:30.9 7.7 $ 0.62 \pm 0.37$ $ \le -0.48$ 7.8$~\pm~$ 3.6 299.9 -10.94
140 RXJ1919.4-4031 19:19:29.1 -40:31:34.7 9.0 $-0.02 \pm 0.40$ $ 0.51 \pm 0.56$ 12.1$~\pm~$ 4.4 209.3 -11.09
141 RXJ1919.5-3639 19:19:31.5 -36:39:37.2 9.4 $-0.96 \pm 0.51$ $ \le 0.61$ 8.3$~\pm~$ 3.9 298.4 -11.49
142 RXJ1919.9-3924 19:19:55.3 -39:24:56.6 16.5 $-0.40 \pm 0.31$ $ \ge 0.17$ 14.8$~\pm~$ 4.7 306.5 -11.21
143 RXJ1919.9-4009 19:19:59.1 -40:09:22.0 7.5 $-0.52 \pm 0.36$ $-0.43 \pm 0.82$ 10.4$~\pm~$ 4.1 252.7 -11.25
144 RXJ1920.6-3911 19:20:41.4 -39:11:29.6 7.9 $ 0.66 \pm 0.36$ $ 0.35 \pm 0.45$ 7.3$~\pm~$ 3.3 314.8 -10.93
145 RXJ1920.9-3320 19:20:59.0 -33:20:06.7 9.5 $ 0.32 \pm 0.37$ $ 0.12 \pm 0.45$ 10.4$~\pm~$ 4.0 257.8 -11.00
146 RXJ1921.1-4002 19:21:09.2 -40:02:14.4 9.6 $ \le -0.55$   8.6$~\pm~$ 4.1 264.9 -11.52
147 RXJ1921.4-3459 19:21:28.9 -34:59:04.4 472.1 $-0.10 \pm 0.07$ $-0.04 \pm 0.11$ 202.2$~\pm~$14.9 300.4 -11.11
148 RXJ1922.0-3549 19:22:01.8 -35:49:16.1 9.8 $ \ge 0.54$ $-0.72 \pm 0.33$ 7.8$~\pm~$ 4.0 311.7 -10.87
149 RXJ1922.4-3806 19:22:24.3 -38:06:13.6 8.3 $ \ge 0.60$ $-0.06 \pm 0.45$ 6.7$~\pm~$ 3.4 303.9 -10.87
150 RXJ1922.9-3545 19:22:55.3 -35:45:39.2 21.4 $ \ge 0.68$ $ \ge 0.53$ 10.5$~\pm~$ 3.9 303.9 -10.87
151 RXJ1923.3-3658 19:23:18.9 -36:58:39.3 9.7 $-0.05 \pm 0.37$ $ 0.30 \pm 0.56$ 10.2$~\pm~$ 4.0 320.7 -11.10
152 RXJ1923.6-3551 19:23:37.6 -35:51:39.8 8.7 $ \ge 0.41$ $ 0.48 \pm 0.47$ 6.2$~\pm~$ 3.2 298.5 -10.87
153 RXJ1923.8-3700 19:23:51.9 -37:00:08.2 7.6 $ 0.51 \pm 0.34$ $-0.02 \pm 0.51$ 7.4$~\pm~$ 3.3 311.9 -10.96
154 RXJ1923.8-4036 19:23:53.3 -40:36:46.4 66.9 $-0.08 \pm 0.19$ $-0.35 \pm 0.27$ 33.1$~\pm~$ 6.3 275.6 -11.10
155 RXJ1924.1-3333 19:24:09.9 -33:33:10.2 8.0 $ 0.74 \pm 0.40$ $ 0.32 \pm 0.42$ 9.7$~\pm~$ 4.2 296.8 -10.91
156 RXJ1924.3-4008 19:24:20.2 -40:08:35.5 7.7 $ 0.02 \pm 0.46$ $ \le -0.11$ 10.0$~\pm~$4.3 309.0 -11.08
157 RXJ1924.4-3959 19:24:27.9 -39:59:29.1 10.3 $ 0.53 \pm 0.38$ $ 0.87 \pm 0.32$ 6.9$~\pm~$ 3.2 307.9 -10.95
158 RXJ1924.5-3442 19:24:34.0 -34:42:34.6 20.5 $-0.29 \pm 0.31$ $ 0.95 \pm 0.47$ 15.0$~\pm~$ 4.5 298.9 -11.17
159 RXJ1924.7-3601 19:24:47.3 -36:01:15.1 7.5 $-0.09 \pm 0.45$ $ 0.20 \pm 0.77$ 7.7$~\pm~$ 3.5 297.7 -11.11
160 RXJ1925.0-3621 19:25:02.7 -36:21:39.1 10.1 $ 0.07 \pm 0.40$ $-0.22 \pm 0.54$ 8.2$~\pm~$ 3.4 297.3 -11.06
161 RXJ1925.0-3549 19:25:03.9 -35:49:34.4 7.6 $ \ge 0.39$ $ 0.60 \pm 0.32$ 10.8$~\pm~$ 4.6 297.0 -10.87
162 RXJ1925.3-3413 19:25:21.4 -34:13:06.4 7.4 $ \le -0.49$ $ \le 0.88$ 9.6$~\pm~$ 4.3 312.5 -11.52
163 RXJ1926.5-3426 19:26:31.8 -34:26:25.7 7.6 $ \le -0.47$ $ \ge -0.60$ 6.8$~\pm~$ 3.5 300.9 -11.52
164 RXJ1927.1-3713 19:27:06.2 -37:13:42.2 14.6 $ \ge 0.65$ $ 0.77 \pm 0.30$ 10.2$~\pm~$ 4.0 316.9 -10.87
165 RXJ1927.4-3847 19:27:28.0 -38:47:06.9 28.3 $ \ge 0.71$ $ 0.29 \pm 0.25$ 17.3$~\pm~$ 5.0 307.7 -10.87
166 RXJ1927.9-3955 19:27:55.0 -39:55:03.8 7.9 $ \le -0.44$ $ \le 0.98$ 5.5$~\pm~$3.0 325.6 -11.52


Table 2. continued
No. Designation $\alpha _{2000}$ (X-ray) $\delta _{2000}$ ML HR 1 HR 2 Counts Exp. [s] $\log ECF$
167 RXJ1928.0-4050 19:28:04.8 -40:50:04.0 46.2 $ 0.60 \pm 0.17$ $ 0.00 \pm 0.22$ 31.1$~\pm~$ 6.5 322.3 -10.94
168 RXJ1928.2-3352 19:28:13.1 -33:52:16.1 11.9 $ \ge 0.45$ $ 0.03 \pm 0.45$ 8.2$~\pm~$ 3.5 281.6 -10.87
169 RXJ1928.2-3915 19:28:13.3 -39:15:13.5 7.4 $ 0.76 \pm 0.70$ $ \le -0.33$ 5.1$~\pm~$ 3.0 320.8 -10.91
170 RXJ1928.3-4031 19:28:20.6 -40:31:19.7 10.3 $ \ge 0.48$ $ 0.85 \pm 0.54$ 9.4$~\pm~$ 4.4 325.7 -10.87
171 RXJ1928.5-3508 19:28:31.6 -35:08:02.0 268.9 $ 0.83 \pm 0.07$ $ 0.27 \pm 0.11$ 88.8$~\pm~$ 9.9 307.2 -10.90
172 RXJ1928.7-3646 19:28:46.3 -36:46:38.6 13.6 $ \ge 0.52$ $ 0.15 \pm 0.35$ 9.7$~\pm~$ 3.7 308.9 -10.87
173 RXJ1929.0-3805 19:29:03.2 -38:05:15.8 8.6 $ 0.39 \pm 0.57$ $ \ge 0.42$ 7.5$~\pm~$ 4.0 324.6 -10.98
174 RXJ1929.2-4055 19:29:16.0 -40:55:20.4 9.1 $ \le -0.43$   5.4$~\pm~$ 2.8 329.9 -11.52
175 RXJ1929.6-4018 19:29:36.5 -40:18:53.6 39.3 $ 0.80 \pm 0.17$ $ 0.07 \pm 0.23$ 26.9$~\pm~$ 5.9 344.0 -10.90
176 RXJ1929.8-3702 19:29:50.0 -37:02:35.7 14.8 $-0.74 \pm 0.35$ $ \ge -0.03$ 12.9$~\pm~$ 4.6 318.8 -11.36
177 RXJ1929.9-3338 19:29:57.4 -33:38:16.7 8.9 $ \ge 0.38$ $-0.21 \pm 0.43$ 8.5$~\pm~$ 3.9 281.0 -10.87
178 RXJ1930.0-3302 19:30:03.1 -33:02:55.2 7.9 $ \le -0.57$   6.0$~\pm~$ 3.7 248.9 -11.52
179 RXJ1930.6-3525 19:30:39.2 -35:25:47.5 13.8 $ \ge 0.61$ $-0.19 \pm 0.31$ 13.6$~\pm~$ 4.7 324.4 -10.87
180 RXJ1931.1-3441 19:31:08.1 -34:41:06.6 11.0 $ \ge 0.39$ $ \le -0.47$ 9.6$~\pm~$ 4.1 319.5 -10.87
181 RXJ1931.4-4008 19:31:25.1 -40:08:46.9 8.8 $ 0.65 \pm 0.39$ $ 0.72 \pm 0.38$ 6.4$~\pm~$ 3.2 344.1 -10.93
182 RXJ1931.5-3340 19:31:32.5 -33:40:15.9 7.8 $ \le -0.51$   5.8$~\pm~$ 3.3 272.9 -11.52
183 RXJ1931.6-3354 19:31:37.7 -33:54:38.7 96.7 $ 0.93 \pm 0.07$ $ 0.76 \pm 0.10$ 52.5$~\pm~$ 8.4 285.2 -10.88
184 RXJ1932.3-3804 19:32:19.3 -38:04:58.6 7.4 $ \ge 0.41$ $ 0.67 \pm 0.32$ 6.0$~\pm~$ 3.3 324.9 -10.87
185 RXJ1932.5-3506 19:32:33.5 -35:06:32.9 7.8 $ \ge 0.47$ $-0.46 \pm 0.40$ 8.0$~\pm~$ 3.8 313.0 -10.87
186 RXJ1932.5-3837 19:32:34.1 -38:37:00.5 10.6 $ \ge 0.22$ $ \le -0.54$ 6.5$~\pm~$ 3.6 329.6 -10.87
187 RXJ1932.7-3432 19:32:44.3 -34:32:22.7 11.8 $-0.34 \pm 0.31$ $ 0.50 \pm 0.63$ 13.4$~\pm~$ 4.6 305.7 -11.19
188 RXJ1932.7-3858 19:32:45.6 -38:58:39.6 9.5 $ 0.88 \pm 0.54$ $ \le -0.45$ 7.4$~\pm~$ 3.6 336.0 -10.89
189 RXJ1932.9-3554 19:32:56.0 -35:54:23.0 7.9 $ \ge 0.30$ $ \le -0.13$ 5.6$~\pm~$ 3.2 314.9 -10.87
190 RXJ1933.2-3337 19:33:18.1 -33:37:29.4 10.5 $ 0.55 \pm 0.50$ $ \ge 0.26$ 8.8$~\pm~$ 3.9 284.4 -10.95
191 RXJ1933.3-3812 19:33:20.2 -38:12:30.8 14.7 $ 0.68 \pm 0.40$ $-0.08 \pm 0.39$ 10.9$~\pm~$ 4.0 350.1 -10.92
192 RXJ1933.5-3743 19:33:33.5 -37:43:46.7 7.4 $ \le -0.58$   5.6$~\pm~$ 3.5 336.1 -11.52
193 RXJ1933.6-3453 19:33:41.6 -34:53:27.1 11.8 $ 0.77 \pm 0.34$ $ 0.48 \pm 0.37$ 13.2$~\pm~$ 4.7 321.7 -10.91
194 RXJ1933.8-3522 19:33:51.3 -35:22:53.1 7.6 $-0.29 \pm 0.47$ $ \le -0.03$ 9.0$~\pm~$ 3.9 320.6 -11.17
195 RXJ1934.5-3620 19:34:33.6 -36:20:43.0 9.0 $ \ge 0.51$ $ 0.06 \pm 0.42$ 6.8$~\pm~$ 3.7 318.2 -10.87
196 RXJ1934.6-3433 19:34:41.1 -34:33:33.2 7.7 $ \le -0.40$   9.0$~\pm~$ 4.2 328.1 -11.52
197 RXJ1934.7-3805 19:34:46.7 -38:05:06.0 52.9 $ 0.76 \pm 0.18$ $ 0.26 \pm 0.20$ 30.8$~\pm~$ 6.3 342.6 -10.91
198 RXJ1935.5-3536 19:35:34.2 -35:36:10.9 9.9 $ 0.42 \pm 0.47$ $ 0.87 \pm 0.57$ 8.3$~\pm~$ 3.5 329.8 -10.98
199 RXJ1936.0-3325 19:36:03.6 -33:25:59.1 8.8 $ 0.89 \pm 0.38$ $ \ge 0.16$ 4.5 $~\pm~$2.7 274.4 -10.88
200 RXJ1936.0-4002 19:36:05.6 -40:02:24.6 10.7 $-0.21 \pm 0.39$ $ \ge 0.24$ 9.9$~\pm~$ 3.8 335.3 -11.14
201 RXJ1936.9-3429 19:36:56.9 -34:29:28.0 9.4 $ 0.28 \pm 0.42$ $ \le -0.44$ 8.7$~\pm~$ 3.8 305.6 -11.01
202 RXJ1937.2-3958 19:37:12.6 -39:58:01.1 22.1 $ 0.41 \pm 0.26$ $ 0.21 \pm 0.29$ 21.6$~\pm~$ 5.6 333.6 -10.98
203 RXJ1937.2-4010 19:37:13.2 -40:10:21.5 11.8 $ \ge 0.46$ $ 0.08 \pm 0.44$ 8.8$~\pm~$ 4.0 335.8 -10.87
204 RXJ1938.0-3801 19:38:03.0 -38:01:05.8 10.3 $ 0.04 \pm 0.49$ $ \ge 0.46$ 7.7$~\pm~$ 3.6 346.1 -11.07
205 RXJ1938.1-3914 19:38:09.4 -39:14:02.4 9.3 $ \ge 0.36$ $ \ge 0.42$ 3.6$~\pm~$ 2.6 345.0 -10.87
206 RXJ1938.2-4006 19:38:13.1 -40:06:38.1 7.8 $ 0.55 \pm 0.40$ $ \ge 0.50$ 7.6$~\pm~$4.0 333.7 -10.95

The moderate energy resolution of the PSPC allows to extract some spectral information from the RASS data, namely so-called hardness ratios, i.e., X-ray colors, which are defined as follows: If Zs,h1,h2 are the count rates in the bands soft, hard 1, and hard 2, respectively, then

 \begin{displaymath}%
HR~1~=~\frac{ Z_{h1} + Z_{h2} - Z_{s} } { Z_{h1} + Z_{h2} +...
... \quad
HR~2~=~\frac{ Z_{h2} - Z_{h1} } { Z_{h2} + Z_{h1}}\cdot
\end{displaymath} (1)

I.e., hardness ratios range from -1 to +1, hardness ratio errors can be larger than 2. If no counts are detected, e.g, in the soft band, then HR 1 = 1, but one can estimate a lower limit to HR 1 by using the upper limit to the soft band count rate $Z_{\rm s}$ in Eq. (1), similar for upper limits to HR 1 as well as for upper and lower limits to HR 2.

In Table 2, we list all RASS X-ray sources detected in our study area with X-ray position, likelihood for existence, hardness ratio, number of counts, exposure time, and individual energy conversion factor

 \begin{displaymath}%
ECF = \left( 5.30 \cdot HR~1 + 8.31 \right) \cdot 10 ^{-12}~{\rm erg~cm} ^{-2}~{\rm cts}^{-1}
\end{displaymath} (2)

according to Schmitt et al. (1995).

In Table 3, we list the optical counterparts to the X-ray sources, most of which are the closest counterparts, but in four cases, the most likely counterpart turned out to be not the closest potential optical counterpart. Table 3 gives optical positions, offsets between X-ray and optical positions, V magnitudes, X-ray to optical flux ratios, identification information, e.g. whether it is a new young star, and remarks, e.g. on previously known stars found among our X-ray sources. The typical positional error of RASS sources is 40 arcsec (Neuhäuser et al. 1995), which we allow as offset between optical and X-ray position for source identification. We searched for stellar counterparts in Simbad, the Hubble Space Telescope Guide Star Catalog (GSC), and the NASA Extragalactic Database (NED). We list in Table 3 the optical positions, V magnitude, X-ray to optical flux ratio, as well as some more information on the identified counterparts. See Sect. 3 for details on the identification. For calculating the X-ray to optical flux ratio, we use

 \begin{displaymath}%
f_{V} = 10 ^{ -0.4 \cdot (V + 13.42) }~{\rm erg~cm} ^{-2}~{\rm s} ^{-1}
\end{displaymath} (3)

(with V in ${\rm mag}$) and the X-ray flux, which we get from the data in Table 2 via

 \begin{displaymath}%
f_{\rm X} = ECF \cdot {\rm counts}/{\rm exposure}.
\end{displaymath} (4)

For sources where we can list only an upper or lower limit to HR 1 (in Table 2), we use HR 1 = 1 or HR 1 = -1, respectively, for calculating the flux according to Eq. (2). The X-ray to optical flux ratio already gives some hints on the nature of an unidentified X-ray source: Extragalactic X-ray sources are optically faint but X-ray bright with $\log (f_{\rm X}/f_{V})~\ge~-0.5$, while normal stars usually have $\log (f_{\rm X}/f_{V})~\le~-1$ (Stocke et al. 1983; Motch et al. 1998).


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