Other
Scientific paper
May 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19...29k&link_type=abstract
Advances in Space Research, Volume 19, Issue 1, p. 29-34.
Other
Scientific paper
Three bright X-ray transient sources GRO J0422+32, GRS 1009-45 and GRS 1716-24 detected in 1992-1993 continue the sequence of such transient sources which were observed by the broad-band MIR-KVANT X-ray observatory in the period since 1988. Two of them, GRO J0422+32 and GRS 1716-29, may be classified as hard X-ray novae where the X-ray spectrum formation is probably dominated by comptonization, GRS 1009-45 is a typical soft X-ray nova with a strong soft thermal component and hard power-law tail. In this paper the results of broad-band (from 2 to 200-500 keV) spectroscopy for these sources are presented and are compared to earlier observations of other X-ray novae.
Aleksandrovich N. L.
Arefiev Vadim A.
Borkous V. V.
Borozdin Konstantin N.
Brinkman Albert C.
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