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Physical mechanisms in stellar pulsations
The Journal of the Acoustical Society of America, 1985Stars evolve from their births to their deaths by converting their store of hydrogen to helium, and then much of this helium is fused to heavier elements such as carbon, oxygen, and up to iron. During this evolution, the stellar mass may decrease by a stellar wind mass loss, the radius usually greatly increases, and the radiation luminosity emitted at ...
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Nonradial and Nonlinear Stellar Pulsation
1980Observational evidence of radial mode resonances and of nonspherical symmetry in some variable stars of ? Scuti and related types.- ? Scuti variables: The link between giant- and dwarf-type pulsators.- Nonlinear calculations for bump Cepheids.- A nonlinear study of AI Velorum.- Nonlinear ?
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Spherical quasi-newtonian stellar pulsations in RTG
Theoretical and Mathematical Physics, 1996zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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Excitation of Stellar Pulsations
2012In this review I present an overview of our current understanding of thephysical mechanisms that are responsible for the excitation of pulsations in stars withsurface convection zones. These are typically cooler stars such as the Delta Scuti stars,and stars supporting solar-like oscillations.
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