Development of convective instability in a rotating gaseous disk

Details Development of convective instability in a rotating gaseous disk Development of convective instability in a rotating gaseous disk

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986zhpmr..44..163n&link_type=abstract

(ZHETF Pis'ma v Redaktsiiu, vol. 44, Aug. 25, 1986, p. 163-166) JETP Letters (ISSN 0021-3640), vol. 44, Aug. 25, 1986, p. 208-21

Physics

Galactic Evolution, Gas Dynamics, Rotating Fluids, Spiral Galaxies, Convective Flow, Modal Response, Rotary Stability, Topology

Scientific paper

A mechanism by which a spiral structure is formed in a gravitating
rotating gaseous disk is analyzed. Caused by a nonlinear development of
the convective instability, this mechanism may be responsible for the
origin of spiral galaxies.

Affiliated with

Also associated with

No associations

Rating

Development of convective instability in a rotating gaseous disk 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 Development of convective instability in a rotating gaseous disk, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Development of convective instability in a rotating gaseous disk will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-896165