Table 2:
The number of sources from each of the major classes
detected by ISGRI are listed for new (
IGRs) and previously-known
sources. Miscellaneous (Misc.) sources are Galactic objects that are not X-ray binaries (e.g. CVs, SNRs, AXPs, etc.) and Uncl. refers to the group of sources that have yet to be classified.
| |
HMXBs |
LMXBs |
AGN |
Misc. |
Uncl. |
Total |
| IGRs |
32 (15%) |
6 (3%) |
50 (23%) |
15 (7%) |
111 (52%) |
214 |
| previously-known |
46 (16%) |
76 (27%) |
113 (40%) |
32 (11%) |
18
(6%) |
285 |
| Total |
78 (16%) |
82 (16%) |
163 (33%) |
47 (9%) |
129 (26%) |
499 |
Source LaTeX |
All tables |
In the text