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Planets and brown dwarfs around A–F main-sequence stars: performances of radial-velocity surveys with HARPS and first detections
Published online by Cambridge University Press: 06 January 2010
Abstract
Due to their high vsini, early-type main-sequence stars have been considered as unsuitable targets for radial-velocity surveys. Knowing about the presence of planets around those stars is however a key issue to understand the impact of the mass of the central star on the way planets form and evolve. We developped in recent years a method that allows to search for planets around those stars and started radial-velocity surveys focused on these targets. We report here some results obtained so far in terms of performances and detection.
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- © EAS, EDP Sciences, 2010
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