X-Ray Observations of GRS 1915+105
Astrophysics
2019-08-17 v1
Abstract
A comparison of ROSAT observations with simultaneous BATSE monitoring data shows a different intensity evolution in the soft and hard X-ray band of GRS 1915+105 since 1992. In addition, fits of simultaneous ROSAT/BATSE spectra require more than one spectral component. A short description of results of RXTE pointed observations of GRS 1915+105 since April 1996 is also presented.
Keywords
Cite
@article{arxiv.astro-ph/9609099,
title = {X-Ray Observations of GRS 1915+105},
author = {J. Greiner and B. A. Harmon and W. S. Paciesas and E. H. Morgan and R. A. Remillard},
journal= {arXiv preprint arXiv:astro-ph/9609099},
year = {2019}
}
Comments
to appear in "Accretion Phenomena and Associated Outflows", IAU Coll. 163, Port Douglas, Australia, July 1996; 2 pages LATEX with paspconf style file, including 2 ps-figures