Linear oscillations of isotropic stellar systems. II - Radial modes of energy-truncated models

Details Linear oscillations of isotropic stellar systems. II - Radial modes of energy-truncated models Linear oscillations of isotropic stellar systems. II - Radial modes of energy-truncated models

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...147...61s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 147, no. 1, June 1985, p. 61-66.

Astronomy and Astrophysics

Astrophysics

11

Energy Distribution, Equilibrium Equations, Isotropic Media, Linear Vibration, Radial Distribution, Stellar Oscillations, Stellar Systems, Density Wave Model, Eigenvalues, Liouville Equations, Perturbation Theory, Stellar Models

Scientific paper

The Wooley (1954) and Michie-King (respectively 1963, 1967) models are among the examples analyzed in the present solution of the eigenvalue problem for the first-order radial perturbation of four energy-truncated distributions in model stellar systems. All eigenvalues obtained for all models with finite masses and radii are real, and there is no indication of instability in dynamical time scales.

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