Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.264t&link_type=abstract
Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:
Astronomy and Astrophysics
Astrophysics
Scientific paper
I present the main points of the Bulk motion inflow Comptonization Theory and the analysis of the high-energy radiation from black hole transients, using archival data obtained primarily with the Rossi X-ray Timing Explorer (RXTE), and a comprehensive test of the bulk motion Comptonization (BMC) model for the high-soft state continuum. The emergent spectra of over 30 separate measurements of GRO J1655-40, GRS 1915+105, GRS 1739-278, 4U 1630-47, XTE J1755-32, and EXO 1846-031 spectra are successfully fitted by the BMC model, which has been derived from basic physical principles in previous work. This provides direct physical insight into the innermost observable regions where matter impinging upon the event horizon can effectively be directly viewed.
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