Hostname: page-component-76fb5796d-45l2p Total loading time: 0 Render date: 2024-04-30T04:55:23.008Z Has data issue: false hasContentIssue false
  • English
  • Français

Doppler ground-based asteroseismology of the exoplanets host star μ Arae

Published online by Cambridge University Press:  05 January 2006

M. Giard ,
F. Casoli ,
F. Paletou ,
M. Bazot ,
F. Bouchy ,
S. Vauclair  and
N. C. Santos
M. Bazot
Affiliation:
Observatoire Midi-Pyrénées, 14 Av. E. Belin, 31400 Toulouse, France
F. Bouchy
Affiliation:
Laboratoire d'Astrophysique de Marseille, Traverse du Siphon, 13013 Marseille, France
S. Vauclair
Affiliation:
Observatoire Midi-Pyrénées, 14 Av. E. Belin, 31400 Toulouse, France
N. C. Santos
Affiliation:
Centro de Astrofisica da Universidade de Lisbo, Tapada da Ajuda, 1349-018 Lisboa, Portugal
Get access

Abstract

We present here a new result of ground-based asteroseismology obtained with the spectrograph HARPS. The exoplanets host star μ Arae was observed during an 8 nights campaign in order to understand the origin of the overmetallicity of planet-hosting stars. Thanks to very high precision Doppler measurements, we identified more than 20 p-modes in this star and compared it with different models. These results demonstrate the potential of ground-based Doppler asteroseismology and should be considered to be implemented in Dome C in the future in order to benefit of long and uninterrupted observations.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 14: Dome C Astronomy and Astrophysics Meeting , 2005 , pp. 349 - 354
Copyright
© EAS, EDP Sciences, 2005

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)