Variability in Quiescent Black Holes

Details Variability in Quiescent Black Holes Variability in Quiescent Black Holes

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002xrb..confe..13h&link_type=abstract

X-ray Binaries in the Chandra and XMM-Newton Era (with an emphasis on Targets of Opportunity), Abstracts of the conference held

Physics

Quiescent/Low-Luminosity X-Ray Binaries

Scientific paper

Multiwavelength studies of Galactic black holes have focussed upon X-ray bright states when high quality data can be obtained. However, with the advent of Chandra and XMM, and the increased availability of large optical telescopes, we can also study properties of the quiescent state, such as variability in some detail. I will discuss what is known about variability in the quiescent state at different energies, possible origins for it, and what may be learned with multiwavelength studies.

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