arXiv · astro-ph/9801220
Disk and Coronal Instabilities in GRS 1915+105
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Jean Swank, Xingming Chen, Craig Markwardt, Ronald Taam. 1998-01-23. Disk and Coronal Instabilities in GRS 1915+105. https://doi.org/10.1063/1.55914
Cite the original work for its findings. Save a collection to share your selection of sources.