Kappa-Mechanism Excitation of Retrograde Mixed Modes in B-Type Stars

Details Kappa-Mechanism Excitation of Retrograde Mixed Modes in B-Type Stars Kappa-Mechanism Excitation of Retrograde Mixed Modes in B-Type Stars

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..512t&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

Scientific paper

The stability of retrograde mixed modes in rotating B-type stars is
investigated. It is found that these modes are susceptible to
κ-mechanism excitation, due to the iron opacity bump at log T ≈
5.3. The findings are discussed in the context of the pulsation of SPB
and Be stars.

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