Advertisement

Stellar Pulsations and Stability

  • G. S. Bisnovatyi-Kogan
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

Being a dynamical system, the star has diverse oscillatory eigenmodes. When account is taken of thermal processes, some of these appear to be unstable. The increment of such an instability γ, equal to the inverse time scale of the amplitude increase by a factor of e, is usually well below the pulsational frequency ω. Other modes can be unstable in the adiabatic approximation as well, as in the case of convective instability (9.1.2b), for dS/dr < 0.

Keywords

Massive Star Oscillation Cycle Stellar Mass Radial Oscillation Phase Core 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

Copyright information

© Springer-Verlag Berlin Heidelberg 2002

Authors and Affiliations

  • G. S. Bisnovatyi-Kogan
    • 1
  1. 1.Space Research InstituteRussian Academy of SciencesMoscowRussia

Personalised recommendations