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ASCA X-ray observations of the Galactic bulge source SLX 1735-269
| Content Provider | Semantic Scholar |
|---|---|
| Author | David, P. Goldwurm, Andrea Murakami, Toshio Laurent, Ph. M. Goldoni, Paolo Bassini, Via |
| Copyright Year | 1997 |
| Abstract | SLX 1735 269 is among the 10 persistent, high en- ergy, SIGMA sources which contribute signicantly to the last ve year averaged /X-ray emission from the direction of the Galactic Center. Detailed study of the source has only been car- ried out recently from data collected by SIGMA in the 35-150 keV range without successfully establishing the nature of SLX 1735 269, consequently observations with ASCA from 0.6-10 keV were performed with the aim of determining the nature of this source. The spectrum of SLX 1735 269 can be described by a powerlaw-absorber model, of photon index 2. No pe- riodwasdeterminedfromthedatabyepochfoldingintherange 10 to 1000 s nor from a power spectrum analysis in the range 125 ms to 64 s and upper limits to pulsation are derived. Yet the nature of SLX 1735 269 remains to be determined. |
| Starting Page | 229 |
| Ending Page | 233 |
| Page Count | 5 |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | http://aa.springer.de/papers/7322001/2300229.pdf |
| Volume Number | 322 |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |
