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An AD HOC Hypothesis on the Pulsation of Delta Scuti Stars

Published online by Cambridge University Press:  12 April 2016

E. Antonello
E. Antonello*
Affiliation:
Osservatorio Astronomico di Milano-Merate, Italy

Extract

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Taking into account the possible influence of external factors such as the orbital motion in binary systems and the rotational velocity on the pulsation of δScuti stars, it may be possible to explain some properties of these variables.

Type
Part I: Evolution of Stars in the Post-Main Sequence Stage
Information
International Astronomical Union Colloquium , Volume 69: Binary and Multiple Stars as Tracers of Stellar Evolution , 1982 , pp. 33 - 35
Copyright
Copyright © Reidel 1982

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