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Pulsations and chemical composition of main sequence magnetic stars

  • Sylvie Vauclair
  • Noël Dolez
Part VI Seismology of Stars
Part of the Lecture Notes in Physics book series (LNP, volume 367)

Abstract

This paper is a discussion of the present situation concerning the abundance anomalies in Ap Stars as possible catalysts of pulsations through the к-mechanism. A preliminary model is suggested, which is part of a work in progress, in collaboration with D. Gough.

Keywords

Magnetic Pole Stellar Wind Magnetic Axis Magnetic Equator Monthly Notice 
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.

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Copyright information

© Springer-Verlag 1990

Authors and Affiliations

  • Sylvie Vauclair
    • 1
  • Noël Dolez
    • 1
    • 2
  1. 1.Observatoire Midi-PyrénéesToulouseFrance
  2. 2.C.E.R.F.A.C.S.ToulouseFrance

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