G. Houdek
Published 2011-12-30Version 1
In this review I present an overview of our current understanding of the physical mechanisms that are responsible for the excitation of pulsations in stars with surface convection zones. These are typically cooler stars such as the Delta Scuti stars, and stars supporting solar-like oscillations.
Comments: Invited paper to be published in: Proc. 61st Fujihara Seminar "Progress in solar/stellar physics with helio- and asteroseismology", Shibahashi H., ed., Hakone, 12 pages, 6 figures
Poetry in Motion: Asteroseismology of Delta Scuti Stars in Binaries using Kepler Data
Comparing the asteroseismic properties of pulsating pre-extremely low mass white dwarf and delta Scuti stars
Pulsation frequency distribution in Delta Scuti stars
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