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Stellar Evolution, Particle Transport, and the CP Phenomenon

Published online by Cambridge University Press:  14 August 2015

G. Michaud  and
J. Richer
G. Michaud
Affiliation:
Département de physique, Université de Montréal, Montréal, Canada, H3C 3J7
J. Richer
Affiliation:
CERCA, Bureau 400, 5160 Boul. Décarie, Montréal, Canada

Extract

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In the light of recent results from helioseismology, the abundance anomalies seen at the surface of Bp, Ap, Am and Fm stars appear as the measurable superficial effect of a process that has much more general impact.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 667 - 670
Copyright
Copyright © Kluwer 1998

References

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