RXTE Spectroscopy of GRS 1915+105

Details RXTE Spectroscopy of GRS 1915+105 RXTE Spectroscopy of GRS 1915+105

1998-06-24

arxiv.org/abs/astro-ph/9806323v1

New Astron.Rev. 42 (1998) 597-600

Astronomy and Astrophysics

Astrophysics

4 pages LATEX + 1 ps-figure, newarcrc.sty style file; Proc. of 2nd workshop on Galactic Sources with Relativistic Jets; Milton

Scientific paper

10.1016/S1387-6473(98)00079-7

The galactic superluminal motion source GRS 1915+105 has been extensively observed with the RXTE satellite over the last two years. More than 250 RXTE pointings have been performed until mid-May 1998 with more than 1.5 Msec exposure time on roughly a weekly basis. Here we report on first results of our spectral analysis of a major part of these pointed RXTE observations. We establish the existence of at least 5 spectral components and present the changes of these components over the last two years.

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