Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-12-15
Astronomy and Astrophysics
Astrophysics
Invited lecture: X-Ray Timing 2003: Rossi and Beyond (Harvard, 2003)
Scientific paper
10.1063/1.1780993
In all the microquasars with two hHz QPOs, the ratio of the frequencies is 3:2, supporting our suggestion that a non-linear resonance between two modes of oscillation in the accretion disk plays a role in exciting the observed modulations of the X-ray flux. We discuss the evidence in favor of this interpretation, and we relate the black hole spin to the frequencies expected for various types of resonances that may occur in nearly Keplerian disks in strong gravity. For those microquasars where the mass of the central X-ray source is known, the black hole spin can be deduced from a comparison of the observed and expected frequencies.
Abramowicz Marek A.
Kluzniak Wlodzimierz
No associations
LandOfFree
Interpreting black hole QPOs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Interpreting black hole QPOs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interpreting black hole QPOs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-510710