Stellar models under homoaxial rotation - Eulerian equations and simulation of non-uniformly rotating stars

Details Stellar models under homoaxial rotation - Eulerian equations and simulation of non-uniformly rotating stars Stellar models under homoaxial rotation - Eulerian equations and simulation of non-uniformly rotating stars

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.120...43g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 120, no. 1, March 1986, p. 43-59.

Statistics

Computation

Computational Astrophysics, Euler Equations Of Motion, Stellar Models, Stellar Rotation, Computerized Simulation, Polytropic Processes

Scientific paper

The Eulerian equations are set up for a model subject to homoaxial
rotation and suitable for simulation of a non-uniformly rotating star.
These equations are formulated in a non-inertial frame of reference,
rotating uniformly, (i.e., rigidly) with respect to the inertial common
frame.

Affiliated with

Also associated with

No associations

Rating

Stellar models under homoaxial rotation - Eulerian equations and simulation of non-uniformly rotating 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 Stellar models under homoaxial rotation - Eulerian equations and simulation of non-uniformly rotating stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar models under homoaxial rotation - Eulerian equations and simulation of non-uniformly rotating stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1280424