Trapping of Non-Axisymmetric g-Mode Oscillations in Thin Relativistic Disks and kHz QPOs

Details Trapping of Non-Axisymmetric g-Mode Oscillations in Thin Relativistic Disks and kHz QPOs Trapping of Non-Axisymmetric g-Mode Oscillations in Thin Relativistic Disks and kHz QPOs

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pasj...53l..37k&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.53, No. 5, pp.L37-L39

Astronomy and Astrophysics

Astronomy

29

Accretion, Accretion Disks, Quasi-Periodic Oscillations, Relativity, Trapped Oscillations, X-Rays: Stars

Scientific paper

We suggest that in the inner part of geometrically thin relativistic
disks there are trapped non-axisymmetric g-mode oscillations which are
excited by a corotation resonance. These oscillation modes would be the
cause of quasi-periodic kHz oscillations observed in some low-mass X-ray
sources.

Affiliated with

Also associated with

No associations

Rating

Trapping of Non-Axisymmetric g-Mode Oscillations in Thin Relativistic Disks and kHz 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 Trapping of Non-Axisymmetric g-Mode Oscillations in Thin Relativistic Disks and kHz QPOs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Trapping of Non-Axisymmetric g-Mode Oscillations in Thin Relativistic Disks and kHz QPOs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1006958