Discoseismic Modes in Accretion Disks: Effect of the Corotation Resonance

Details Discoseismic Modes in Accretion Disks: Effect of the Corotation Resonance Discoseismic Modes in Accretion Disks: Effect of the Corotation Resonance

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.4302t&link_type=abstract

American Astronomical Society, HEAD meeting #11, #43.02; Bulletin of the American Astronomical Society, Vol. 41, p.731

Astronomy and Astrophysics

Astronomy

Scientific paper

We discuss the stability of various discoseismic modes of black hole accretion disks. In particular the damping and growth of each mode due to the absorption at the corotation radius (where the pattern rotation rate equals the fluid rotation rate) is considered. Unstable modes may be of interest as possible sources for High Frequency QPOs observed in X-ray binaries.

Affiliated with

Also associated with

No associations

Rating

Discoseismic Modes in Accretion Disks: Effect of the Corotation Resonance 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 Discoseismic Modes in Accretion Disks: Effect of the Corotation Resonance, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discoseismic Modes in Accretion Disks: Effect of the Corotation Resonance will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1094975