Detection of the A1742-294 X-Ray Burster above 35 keV
Abstract
A transient hard state of the A1742-294 X-ray burster was detected by Granat/SIGMA in the course of Fall 1992 observations of the Galactic center (GC) region. During the previous five sets of GC observations in 1990-1992, the flux above 35 keV was below the SIGMA detection limit. The spectrum observed in Fall 1992 in the 35-200 keV band can be approximated by the emission of optically thin plasma with temperature Te approximately 40 keV, much higher than Te approximately 8 keV derived from the observations in the standard X-ray band by Granat/ART-P in 1990. Nevertheless, the spectrum of A1742-294 remains significantly softer than that of the nearby black hole candidate 1E 1740.7-2942.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- April 1995
- DOI:
- Bibcode:
- 1995ApJ...443..341C
- Keywords:
-
- Emission Spectra;
- Plasma Spectra;
- X Ray Astronomy;
- X Ray Spectra;
- X Ray Stars;
- X Rays;
- Black Holes (Astronomy);
- Flux (Rate);
- Galactic Bulge;
- X Ray Telescopes;
- Astronomy;
- STARS: INDIVIDUAL ALPHANUMERIC: A1742-294;
- X-RAYS: BURSTS;
- X-RAYS: STARS