Stellar models under homoaxial rotation: Eulerian equations and simulation of non-uniformly rotating stars (Q1085992)
From MaRDI portal
 | This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Stellar models under homoaxial rotation: Eulerian equations and simulation of non-uniformly rotating stars |
scientific article; zbMATH DE number 3984638
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Stellar models under homoaxial rotation: Eulerian equations and simulation of non-uniformly rotating stars |
scientific article; zbMATH DE number 3984638 |
Statements
Stellar models under homoaxial rotation: Eulerian equations and simulation of non-uniformly rotating stars (English)
0 references
1986
0 references
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.
0 references
Eulerian equations
0 references
homoaxial rotation
0 references
non-uniformly rotating star
0 references
non- inertial frame of reference
0 references
