On the uniqueness of motion of viscous gaseous stars

Details On the uniqueness of motion of viscous gaseous stars On the uniqueness of motion of viscous gaseous stars

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mmas...13..391s&link_type=abstract

Mathematical Methods in the Applied Sciences (ISSN 0170-4214), vol. 13, Nov. 1990, p. 391-404.

Statistics

Computation

3

Compressible Fluids, Computational Astrophysics, Equations Of Motion, Stellar Motions, Viscous Fluids, Energy Conservation, Newton Theory, Specific Heat

Scientific paper

The existence of solutions of the evolutionary equations of motion of a
star regarded as a compressible viscous fluid with self-gravitation,
bounded by a free surface, has recently been considered by Secchi
(1990). In this paper, the uniqueness of the solutions cited is studied.

Affiliated with

Also associated with

No associations

Rating

On the uniqueness of motion of viscous gaseous stars 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 On the uniqueness of motion of viscous gaseous stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the uniqueness of motion of viscous gaseous stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-841576