THE SOFT GAMMA-RAY SOURCE 1E 1740.7-2942 REVISITED - SIGMA OBSERVATION OF A NEW TRANSIENT ACTIVITY BEYOND 200 KEV

We present results obtained between 1992 September 14 and 1992 Septemb er 23 by the SIGMA coded aperture telescope on board the GRANAT spacec raft, which further demonstrate that the remarkable soft gamma-ray sou rce 1E 1740.7-2942 is indeed subject to repeated outbursts of hard emi ssion. During the single 1992 September 19-20 observation session, the source was found anew to exceed markedly the SIGMA detection limit be yond 200 keV. Such a high energy excess was not apparent during the fo ur previous observation sessions devoted to 1E 1740.7-2942, nor during the next one. During the whole September 1992 observation program, th e spectral shape of the 40-200 keV source emission was found to be qui te similar to that observed when the source emission was in the so cal led standard state previously identified by SIGMA. The spectral shape of the 1992 September 19-20 high energy excess does not differ signifi cantly from that of the high energy outburst observed by SIGMA on 1990 October 13-14, which was suggestive of positron annihilation radiatio n. Together with the SIGMA observations of a high energy excess in Oct ober 1991, this new SIGMA observation confirms that such a hard state is not an exceptional situation, but appears as a strongly variable ph enomenon (by more than a factor 4-5).