Numerical Treatment of Linear and Nonlinear Stellar Pulsations

The linear stability analysis of stellar models poses a linear fourth or sixth order boundary eigenvalue problem. Methods for its numerical solution are reviewed, most of which face severe problems, if the ratio of the thermal and dynamical timescale falls below unity for a significant fraction of t...

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Detalles Bibliográficos
Autor principal:	Glatzel, Wolfgang
Formato:	Objeto de conferencia
Lenguaje:	Inglés
Publicado:	2019
Materias:	Ciencias Astronómicas asteroseismology hydrodynamics methods: numerical stars: mass loss stars: oscillations
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/167721
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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