GRS 1915+105: The X-ray spectrum following a radio flare

Details GRS 1915+105: The X-ray spectrum following a radio flare GRS 1915+105: The X-ray spectrum following a radio flare

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..124h&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 124-128 (2000).

Computer Science

X-Ray Binaries, Black Holes, X-Ray

Scientific paper

We present simultaneous RXTE (PCA and HEXTE) and CGRO (OSSE) spectra of GRS1915+105 following a radio flaring episode. The outcome of the spectral fits, using both a thermal sombrero and a hybrid thermal/nonthermal model, imply a Kerr hole with a large population of relativistic electrons. The radio-infrared excess (over the disk model) may arise from this population, or it could be a relic from major plasmoid ejections or due to frequent ``baby'' blobs. .

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