Iron Line Diagnostics for the Inner Accretion Disc in GRS 1915+105

Details Iron Line Diagnostics for the Inner Accretion Disc in GRS 1915+105 Iron Line Diagnostics for the Inner Accretion Disc in GRS 1915+105

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cnoc.conf...26m&link_type=abstract

The Second National Conference on Astrophysics of Compact Objects, held in Bologna (Italy), September 19 - 21, 2001, p. 26

Astronomy and Astrophysics

Astrophysics

Scientific paper

We found strong and broad iron Kα fluorescent emission in the spectrum of the "microquasar" GRS 1915+105 observed by BeppoSAX on April 19, 1998. We analysed the data of a relatively stable spectral phase, sorted out from the whole observation, by using a fully relativistic model for XSPEC. Considering the innermost emitting orbit as a line profile fitting parameter, we conclude that r1 ~ 40m.

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