SSS Master Table
| Name |
Countrate(1)
(cts/s) |
T(2)
(eV) |
LBol
(erg/s) |
Type |
Period
(days) |
| |
| Galactic Sources |
| RX J0019.8+2156 |
2.0 |
25-37 (wd) |
(3-9)*1037 |
CBSS |
1.0-1.35 |
| RX J0925.7-4758 |
1.0 |
70-75 (wd) |
(3-7)*1035 |
CBSS |
3.55-4.03 |
| GQ Mus |
0.1 |
25-35 (bb) |
(1-2)*1038 |
N |
0.0588 |
| 1E 1339.8+2837 |
0.01-1.1 |
20-45 (bb) |
1.2*1034-1.2*1036 |
|
|
| AG Dra |
0.01-1.0 |
10-15 (bb) |
9.5*1036 |
Sy |
549-554 |
| U Sco |
|
74-76 (wd) |
(8-60)*1036 |
RN |
1.2306 |
| RR Tel |
0.18 |
12 (wd) |
1.3*1037 |
Sy |
|
| V Sge |
0.001-0.02 |
<80 (bb) |
(1-10)*1037 |
CV |
0.514195 |
| V1974 Cyg |
0.03-76 |
30-51 (wd) |
2*1038 |
N |
0.0812 |
| V751 Cyg |
0.039-0.11 |
15 (bb) |
6.5*1036 |
VY Scl |
|
| |
| Large Magellanic Cloud |
| RX J0439.8-6809 |
1.35 |
20-25 (wd) |
(10-14)*1037 |
CBSS |
0.1404 |
| RX J0513.9-6951 |
<0.06-0.2 |
30-40 (bb) |
(0.1-6)*1037 |
CBSS |
0.76278 |
| Nova LMC 1995 |
0.061 |
20-40 (wd) |
1.5*1038 |
N |
|
| RX J0527.8-6954 |
0.004-0.25 |
18-45 (bb) |
(1-10)*1037 |
CBSS |
0.3926 |
| RX J0537.7-7034 |
<0.002-0.02 |
18-70 (bb) |
(0.6-2)*1037 |
CBSS |
0.125 |
| CAL 83 |
<0.035-0.98 |
39-60 (wd) |
<2*1037 |
CBSS |
1.04 |
| CAL 87 |
0.09 |
63-84 (wd) |
(6-20)*1037 |
CBSS |
0.44267 |
| RX J0550.0-7151 |
<0.02-0.9 |
25-40 (bb) |
|
|
|
| |
| Small Magellanic Cloud |
| 1E 0035.4-7230 |
0.33 |
40-50 (wd) |
(0.8-2)*1037 |
CBSS |
0.1719 |
| RX J0048.4-7332 |
0.19-0.33 |
25-45 (wd) |
(1-8)*1038 |
Sy |
|
| 1E 0056.8-7154 |
0.29 |
30-40 (wd) |
2*1037 |
PN |
|
| RX J0058.6-7146 |
<0.001-0.7 |
15-70 (bb) |
2*1036 |
|
|
| |
| Andromeda Galaxy (M31) |
| RX J0037.4+4015 |
0.3*10-3 |
<34 (wd) |
|
|
|
| RX J0038.5+4014 |
0.8*10-3 |
26-37 (wd) |
|
|
|
| RX J0038.6+4020 |
1.7*10-3 |
28-38 (wd) |
|
|
|
| RX J0039.4+4050 |
2.9*10-3 |
49 (wd) |
|
|
|
| RX J0039.6+4054 |
0.4*10-3 |
<36 (wd) |
|
|
|
| RX J0039.7+4030 |
2.0*10-3 |
<38 (wd) |
|
|
|
| RX J0040.0+4100 |
2.0*10-3 |
52-58 (wd) |
|
|
|
| RX J0040.1+4021 |
0.5*10-3 |
>51 (wd) |
|
|
|
| RX J0040.4+4004 |
0.8*10-3 |
28-36 (wd) |
|
|
|
| RX J0040.7+4015 |
1.3*10-3 |
28-38 (wd) |
|
|
|
| RX J0041.5+4040 |
0.3*10-3 |
31-34 (wd) |
|
|
|
| RX J0041.8+4015 |
3.2*10-3 |
45 (wd) |
|
|
|
| RX J0041.8+4059 |
0.5*10-3 |
29-35 (wd) |
|
|
|
| RX J0042.4+4044 |
1.7*10-3 |
28-38 (wd) |
|
|
|
| RX J0042.4+4048 |
0.6*10-3 |
39-62 (wd) |
|
|
|
| RX J0042.6+4043 |
1.6*10-3 |
>55 (wd) |
|
|
|
| RX J0042.6+4159 |
1.8*10-3 |
>63 (wd) |
|
|
|
| RX J0042.8+4115 |
40.1*10-3 |
65 (wd) |
|
|
|
| RX J0043.3+4120 |
6.7*10-3 |
59-62 (wd) |
|
|
|
| RX J0043.5+4207 |
2.2*10-3 |
32-39 (wd) |
|
|
|
| RX J0043.7+4127 |
1.2*10-3 |
46-60 (wd) |
|
|
|
| RX J0043.9+4151 |
0.9*10-3 |
43 (wd) |
|
|
|
| RX J0044.0+4118 |
2.5*10-3 |
32-39 (wd) |
|
|
|
| RX J0044.2+4026 |
7*10-5 |
>69 (wd) |
|
|
|
| RX J0044.4+4200 |
1.2*10-3 |
47-56 (wd) |
|
|
|
| RX J0045.4+4154 |
<10-5-0.03 |
72-73 (wd) |
(5-10)*1037 |
|
|
| RX J0045.4+4219 |
1.2*10-3 |
51-59 (wd) |
|
|
|
| RX J0045.5+4206 |
3.1*10-3 |
35-40 (wd) |
7*1037 |
|
|
| RX J0046.1+4136 |
0.3*10-3 |
>51 (wd) |
|
|
|
| RX J0046.2+4138 |
1.1*10-3 |
29-38 (wd) |
|
|
|
| RX J0046.2+4144 |
2.1*10-3 |
27-38 (wd) |
|
|
|
| RX J0046.3+4238 |
3.1*10-3 |
53-62 (wd) |
|
|
|
| RX J0047.6+4132 |
0.3*10-3 |
>60 (wd) |
|
|
|
| RX J0047.6+4205 |
0.3*10-3 |
<34 (wd) |
|
|
|
| |
| NGC 55 |
| RX J0016.0-3914 |
0.0045 |
23 ± 30 (bb) |
9*1037 |
|
|
(1) Countrates in the ROSAT PSPC corrected for vignetting, i.e. absorbed on-axis countrates. Countrates in the HRI have been converted to PSPC rates using a conversion factor of PSPC/HRI = 7.8 (Greiner et al. 1996)
(2) Temperatures for the M31 sources are the maximum blackbody temperatures derived from the hardness ratios at the appropriate absorbing column (Greiner et al. 1996)
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This page is maintained by Jochen Greiner (jcg@mpe.mpg.de) and Arne Rau (arau@mpe.mpg.de)
last edited: January 27, 2000