Linear Isentropic Oscillations of Stars : Theoretical Foundations
The study of stellar oscillations is the preeminent way to investigate the stability of stars and to interpret their variability. The theory of the linear, isentropic oscillations of isolated gaseous stars, and thus of compressible spherically symmetric equilibrium configurations, has largely been d...
Enregistré dans:
| Auteurs principaux: | , |
|---|---|
| Format: | Livre numérique |
| Langue: | Anglais |
| Publié: |
Berlin, Heidelberg :
Springer Berlin Heidelberg
[20..].
Cham : Springer Nature |
| Édition: | 1st ed. 2010. |
| Collection: | Astrophysics and Space Science Library
371 |
| Accès en ligne: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Note: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Linear isentropic oscillations of stars, theoretical foundations, by Paul Smeyers, Berlin, Springer, 2010, 1 vol. (XIV-473 p.), Astrophysics and space science library, 978-3-642-13029-8 • Linear Isentropic Oscillations of Stars, Texte imprimé, 9783642266126 • Linear Isentropic Oscillations of Stars, Texte imprimé, 9783642130311 |
Table des matières:
- Basic Concepts The Equations Governing Linear Perturbations in a Quasi-Static Star Deviations from the Hydrostatic and Thermal Equilibrium in a Quasi-Static Star Eigenvalue Problem of the Linear, Isentropic Normal Modes in a Quasi-Static Star Spheroidal and Toroidal Normal Modes Determination of Spheroidal Normal Modes: Mathematical Aspects The Eulerian Perturbation of the Gravitational Potential The Variational Principle of Hamilton Radial Propagation of Waves Classification of the Spheroidal Normal Modes Classification of the Spheroidal Normal Modes (continued) Completeness of the Linear, Isentropic Normal Modes N 2(r) Nowhere Negative as Condition for Non-Radial Modes with Real Eigenfrequencies Asymptotic Representation of Low-Degree, Higher-Order p-Modes Asymptotic Representation of Low-Degree and Intermediate-Degree p-Modes Asymptotic Representation of Low-Degree, Higher-Order g +-Modes in Stars Containing a Convective Core Asymptotic Representation of Low-Degree, Higher-Order g +-Modes in Stars Consisting of a Radiative Core and a Convective Envelope High-Degree, Low-Order Modes Period Changes in a Rapidly Evolving Pulsating Star