Numerical simulators of stability in astrophysical problems
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Publication:1194609
DOI10.1007/BF00644202zbMath0775.76139MaRDI QIDQ1194609
Publication date: 13 October 1992
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Cites Work
- The secular variations in the restricted problem's sixth-order theory and stability: An explicit numerical approach
- The secular variations in the restricted problem: An explicit numerical approach
- A second-order perturbation theory for differentially rotating gaseous polytropes
- Structure-distortion of polytropic stars by differential rotation: Third- order perturbation theory
- Dynamics of close binary systems
- Secular variations in the restricted problem: A numerical technique for studying stability of equilibrium solutions
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