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Stochastically excited oscillations in the upper main sequence

Published online by Cambridge University Press:  18 February 2014

Victoria Antoci
Victoria Antoci*
Affiliation:
Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University Ny Munkegade 120, DK-8000 Aarhus C, Denmark email: [email protected]
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Abstract

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Convective envelopes in stars on the main sequence are usually connected only with stars of spectral types F5 or later. However, observations as well as theory indicate that the convective outer layers in hotter stars, despite being shallow, are still effective and turbulent enough to stochastically excite oscillations. Because of the low amplitudes, exploring stochastically excited pulsations became possible only with space missions such as Kepler and CoRoT. Here I review the recent results and discuss among others, pulsators such as δ Scuti, γ Doradus, roAp, β Cephei, Slowly Pulsating B and Be stars, all in the context of solar-like oscillations.

Keywords

stars: oscillationsstars: variables: δ Scutistars: variables: γ Doradusstars: variables: Sun-like starsstars: variables: β Cepheistars: variables: SPB starsstars: variables: Be stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 333 - 340
Copyright
Copyright © International Astronomical Union 2014 

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