Stability of a thin disk with nearly rigid-body rotation

Details Stability of a thin disk with nearly rigid-body rotation Stability of a thin disk with nearly rigid-body rotation

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42..587a&link_type=abstract

Astronomy Reports, Volume 42, Issue 5, September 1998, pp.587-591

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The instability of a rotating gaseous disk immersed in a galaxy or, more generally, in a system with large mass, is considered. Specifically, the existence of an entropy gradient in the gas is assumed, and slow instabilities resulting from this nonuniformity of the medium are selected out for study. It is shown that this type of instability is absent in a perfect gas, but appears in the presence of hysteresis, if a certain inequality holds.

Affiliated with

Also associated with

No associations

Rating

Stability of a thin disk with nearly rigid-body rotation 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 Stability of a thin disk with nearly rigid-body rotation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of a thin disk with nearly rigid-body rotation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-811790