Numerical Simulations Reveal the Origin of QPOs in Black Hole Candidates

Details Numerical Simulations Reveal the Origin of QPOs in Black Hole Candidates Numerical Simulations Reveal the Origin of QPOs in Black Hole Candidates

2005-01-14

arxiv.org/abs/astro-ph/0501299v1

Astronomy and Astrophysics

Astrophysics

6 pages, 7 figures To be published in the Proceedings of 5th Microquasar Conference (Beijing, 2004)

Scientific paper

We present results of various types of numerical simulations of black hole
accretion disks and find that those flows which are relatively non-dissipative
and which contain accretion shocks are the best candidates so far. The power
density spectra (PDS) reveal the aspects which are similar to what are observed
in black hole candidates.

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