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- W2099616905 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." @default.
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- W2099616905 date "1997-06-01" @default.
- W2099616905 modified "2023-10-16" @default.
- W2099616905 title "ASCA X-ray observations of the Galactic bulge source SLX 1735-269" @default.
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