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Solar-Like Oscillations of Procyon A: Stellar Models and Time Series Simulations versus Observations1

Published online by Cambridge University Press:  12 April 2016

C. Barban ,
E. Michel ,
M. Martic ,
J. Schmitt ,
J. C. Lebrun ,
A. Baglin  and
J. L. Bertaux
C. Barban
Affiliation:
Observatoire de Paris, DASGAL, CNRS UMR 8633, 92195 Meudon, France
E. Michel
Affiliation:
Observatoire de Paris, DASGAL, CNRS UMR 8633, 92195 Meudon, France
M. Martic
Affiliation:
Service d’Aéronomie, CNRS, 91371 Verrières le Buisson, France
J. Schmitt
Affiliation:
Service d’Aéronomie, CNRS, 91371 Verrières le Buisson, France
J. C. Lebrun
Affiliation:
Service d’Aéronomie, CNRS, 91371 Verrières le Buisson, France
A. Baglin
Affiliation:
Observatoire de Paris, DESPA, CNRS UMR 8632, 92195 Meudon, France
J. L. Bertaux
Affiliation:
Service d’Aéronomie, CNRS, 91371 Verrières le Buisson, France

Abstract

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The aim of this paper (further developed in Barban et al. 1999) is to present new evidence of the possible stellar origin of the observed excess power in the power spectrum of Procyon A presented in Martic et al. (1999) by comparing these observational data with theoretical predictions and numerical simulations.

Type
Part 6. Variables Close to the Main Sequence
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 461 - 462
Copyright
Copyright © Astronomical Society of the Pacific 2000

Footnotes

1

Based on observations collected at the Observatoire de Haute-Provence (CNRS, France)

References

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