Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-30T01:43:54.339Z Has data issue: false hasContentIssue false

P-Mode Observations on α Cen A with CORALIE

Published online by Cambridge University Press:  12 April 2016

F. Carrier
Affiliation:
Observatoire de Genève, CH-1290 Sauverny, Switzerland
F. Bouchy
Affiliation:
Observatoire de Genève, CH-1290 Sauverny, Switzerland
G. Meynet
Affiliation:
Observatoire de Genève, CH-1290 Sauverny, Switzerland
A. Maeder
Affiliation:
Observatoire de Genève, CH-1290 Sauverny, Switzerland
J. Provost
Affiliation:
Département Cassini, UMR CNRS 6529, Observatoire de la Côte d’Azur, BP 4229, 06304 Nice CEDEX 4, France
G. Berthomieu
Affiliation:
Département Cassini, UMR CNRS 6529, Observatoire de la Côte d’Azur, BP 4229, 06304 Nice CEDEX 4, France
P. Morel
Affiliation:
Département Cassini, UMR CNRS 6529, Observatoire de la Côte d’Azur, BP 4229, 06304 Nice CEDEX 4, France
F. Thévenin
Affiliation:
Département Cassini, UMR CNRS 6529, Observatoire de la Côte d’Azur, BP 4229, 06304 Nice CEDEX 4, France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have made a clear detection of p-mode oscillations in the G2V star α Cen A with the CORALIE spectrograph. The power spectrum clearly shows several identifiable peaks between 1.8 and 2.9 mHz. A preliminary astrophysical interpretation of these p-modes is presented.

Type
Part 4. The Interaction between Convection and Pulsation
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Bouchy, F. & Carrier, F., 2001, A&A, 374, L5 Google Scholar
Morel, P., Provost, J., Lebreton, Y., et al. 2000, A&A, 363, 675 Google Scholar