Detection Of The A1742-294 X-Ray Burster Above 35 Kev

ASTROPHYSICAL JOURNAL(1995)

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Abstract
A transient hard state of the A1742-294 X-ray burster was detected by Granat/SIGMA in the course of 1992 fall 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 1992 fall in the 35-200 keV band can be approximated by the emission of optically thin plasma with temperature T-e similar to 40 keV, much higher than T-e similar to 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.
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Key words
STARS, INDIVIDUAL (A1742 - 294), X-RAYS, BURSTS, X-RAYS, STARS
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