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Multiperiodicity in pulsating red giants

Published online by Cambridge University Press:  12 April 2016

J.R. Percy ,
A.G. Bakos ,
G. Besla ,
D. Hou ,
V. Velocci  and
G.W. Henry
J.R. Percy
Affiliation:
Department of Astronomy & Astrophysics, University of Toronto, Toronto, ON Canada M5S 3H8
A.G. Bakos
Affiliation:
Department of Astronomy & Astrophysics, University of Toronto, Toronto, ON Canada M5S 3H8
G. Besla
Affiliation:
Department of Astronomy & Astrophysics, University of Toronto, Toronto, ON Canada M5S 3H8
D. Hou
Affiliation:
Department of Astronomy & Astrophysics, University of Toronto, Toronto, ON Canada M5S 3H8
V. Velocci
Affiliation:
Department of Astronomy & Astrophysics, University of Toronto, Toronto, ON Canada M5S 3H8
G.W. Henry
Affiliation:
Center of Excellence in Information Systems, Tennessee State University, Nashville TN 37203-3401, USA

Abstract

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We describe several aspects of the variability of bright pulsating red giant (PRG) stars, with emphasis on the determination of pulsation modes and pulsation masses by using observed multiperiodicity and pulsation constants (Q- values). Our studies of bright PRGs provide a model for the analysis and interpretation of the thousands of PRGs being discovered in surveys of Local Group galaxies.

Type
Part 5. Red Giants, Miras, post-AGB stars and proto-planetary nebulae
Information
International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 348 - 352
Copyright
Copyright © Astronomical Society of the Pacific 2004

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