Physical Characteristics of XTE-J1650 and GRS 1915+105 with Bepposax

Details Physical Characteristics of XTE-J1650 and GRS 1915+105 with Bepposax Physical Characteristics of XTE-J1650 and GRS 1915+105 with Bepposax

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1127m&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Computer Science

Scientific paper

We show preliminary results of a comparative spectral and timing analysis of Galactic Black Holes XTE J1650-500 and GRS 1915+105, using data from BeppoSAX. A clear relation is present between the evolution of energy spectra and power spectra. The central frequency of a given QPO is increasing with the softening of the energy spectra. This is consistent with the following picture: the spectral evolution from Hard to Soft is occurring together with a decreasing of the dimension of the Comptonizing corona. This also implies that the effect of bulk inflow vs thermal Comptonization is increasing its importance during the softening of the source.

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