Disk and Coronal Instabilities in GRS 1915+105
Astrophysics
2009-10-30 v1
Abstract
We present time-resolved GRS 1915+105 energy and power spectra observed by RXTE, during an episode where the X-ray intensity makes an extreme dip. If the spectra are modeled in terms of disk and power law components, both have large variations. When the inner disk is disrupted, the power law dominates, exhibiting quasi-periodic oscillations with varying frequency until the inner disk returns.
Keywords
Cite
@article{arxiv.astro-ph/9801220,
title = {Disk and Coronal Instabilities in GRS 1915+105},
author = {Jean Swank and Xingming Chen and Craig Markwardt and Ronald Taam},
journal= {arXiv preprint arXiv:astro-ph/9801220},
year = {2009}
}
Comments
4 pages, 1 figure,to be published in the proceedings of the conference "Accretion Processes in Astrophysics: Some Like it Hot", held at U. Md., October 1997, eds. S. Holt and T. Kallman