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Observation of γ Doradus Stars in the Space Asteroseismology Era

Published online by Cambridge University Press:  12 April 2016

F.M. Zerbi  and
A.B. Kaye
F.M. Zerbi
Affiliation:
INAF - Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate (Lc), Italy
A.B. Kaye
Affiliation:
Applied Physics Division, Los Alamos National Laboratory; X-5, Mail Stop F-663; Los Alamos, New Mexico 87545

Abstract

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Almost 10 years have passed since the first claims of the existence of a new class of slowly pulsating variables near the cool border of δ Scuti instability strip. The consolidated class of γ Doradus variables faces now the challenge of space. In this paper, we review the most recent theoretical and observational results of these stars and we discuss how our knowledge of their nature will benefit from data collected in the forthcoming space-borne asteroseismological missions.

Type
Part 4. The Interaction between Convection and Pulsation
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 494 - 500
Copyright
Copyright © Astronomical Society of the Pacific 2002

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