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Monthly Notices of the Royal Astronomical Society, v. 365, n. 1, p. 327-338, 2006. http://fr.arxiv.org/abs/astro-ph/0510326v1
Astronomy and Astrophysics, v. 419, n. 2, p. 695-701, 2004. http://dx.doi.org/10.1051/0004-6361:20035830
Context. Exoplanet properties crucially depend on the parameters of their host stars: more accurate stellar parameters yield more accurate exoplanet characteristics. When the exoplanet host star shows pulsations, asteroseismology can be used for an improved description of the stellar parameters. Aims: We aim to revisit the pulsational...
We undertook a multisite spectroscopic campaign for the β Cephei star ν Eridani. A total of 2294 high-resolution spectra were obtained from telescopes at 11 different observatories around the world. The time base of dedicated multisite observations is 88 d. To this data set we have added 148 older, previously unpublished spectra, such that the...
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