Linear radial perturbations of supermassive stars

Details Linear radial perturbations of supermassive stars Linear radial perturbations of supermassive stars

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..43..375s&link_type=abstract

Astrophysics and Space Science, vol. 43, Sept. 1976, p. 375-395.

Astronomy and Astrophysics

Astrophysics

2

Dynamic Stability, Numerical Integration, Perturbation Theory, Stellar Models, Astronomical Models, Quasars, Radial Distribution, Stellar Mass, Stellar Radiation, Supergiant Stars

Scientific paper

Numerical integration of the linear nonadiabatic equations for radial perturbations of physical models of supermassive stars confirm the existence of both dynamical and secular instabilities above a critical mass. The value of the latter agrees very well with that deduced from approximate stability criteria. The present analysis demonstrates the existence of a continuous transition between dynamical and secular modes in a sequence of models with different masses.

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