Advection-dominated disks: another standard disk model.

Details Advection-dominated disks: another standard disk model. Advection-dominated disks: another standard disk model.

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996asthe..89..388m&link_type=abstract

Astronomical Herald, Vol. 89, No. 9, p. 388 - 392

Astronomy and Astrophysics

Astronomy

Accretion Disks: Models

Scientific paper

The optically thin, advection-dominated disk model has drawn much attention recently. In advection-dominated disks, potential energy of accreting gas is inefficiently converted to radiation, thereby being advected into a central object. The disk then becomes hot, emitting high-energy radiation. In adddition the disk is thermally unstable, as long as heat diffusion is neglected, so that rapid variability is expected. The authors introduce such an odd disk model.

Affiliated with

Also associated with

No associations

Rating

Advection-dominated disks: another standard disk model. 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 Advection-dominated disks: another standard disk model., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Advection-dominated disks: another standard disk model. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1460013