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Mode Identification in the δ Scuti Star 20 CVn

Published online by Cambridge University Press:  12 April 2016

M. Chadid ,
P. Mathias ,
J. De Ridder  and
C. Aerts
M. Chadid*
Affiliation:
Observatoire de la Côte d’Azur, UMR 6528, Nice, France
P. Mathias
Affiliation:
Observatoire de la Côte d’Azur, UMR 6528, Nice, France
J. De Ridder
Affiliation:
Observatoire de la Côte d’Azur, UMR 6528, Nice, France
C. Aerts
Affiliation:
Observatoire de la Côte d’Azur, UMR 6528, Nice, France
*
1 Postdoctoral Fellow, ESO/Paranal; e-mail: chadid@obs-nice.fr & mchadid@eso.org

Abstract

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We present a new Spectroscopic study of the δ Scuti star 20 CVn in order to solve the controversy on the type of pulsation mode of this object.

Information

Type
Part 2.4. Delta Scuti Stars
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 334 - 335
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Mathias, P., Aerts, C. 1996, A&A, 312, 905 Google Scholar
Roberts, D.H., Lehár, J., & Dreher, J.W. 1987, AJ, 93, 968 CrossRefGoogle Scholar
Rodríguez, E., Rolland, A., Garrido, R., et al. 1998, A&A, 331, 171 Google Scholar
Stellingwerf, R.F. 1978, ApJ, 224, 953 CrossRefGoogle Scholar
Vanicek, P. 1971, Ap&SS, 12, 10 Google Scholar