Numerical modeling of gyroturbulent oscillations of X-ray source luminosity

Details Numerical modeling of gyroturbulent oscillations of X-ray source luminosity Numerical modeling of gyroturbulent oscillations of X-ray source luminosity

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1174k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Nov.-Dec. 1990, p. 1174-1180. In Russian.

Statistics

Computation

1

Accretion Disks, Computational Astrophysics, Luminosity, X Ray Binaries, Astronomical Models, Astronomical Spectroscopy, Stellar Oscillations, Turbulence Effects

Scientific paper

A nonlinear model of disk accretion of an ideal turbulent gas to a massive center is given. A numerical solution of the problem of unsteady rotation of a gas surrounding a compact object is obtained. Strong oscillatory regimes of gyroturbulent rotation are found. It is quite possible that these oscillations are responsible for quasiperiodic variability in luminosity of X-ray sources.

Affiliated with

Also associated with

No associations

Rating

Numerical modeling of gyroturbulent oscillations of X-ray source luminosity 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 Numerical modeling of gyroturbulent oscillations of X-ray source luminosity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical modeling of gyroturbulent oscillations of X-ray source luminosity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1629773