Planets and brown dwarfs around A-F main-sequence stars: performances of radial-velocity surveys with HARPS and first detections

Details Planets and brown dwarfs around A-F main-sequence stars: performances of radial-velocity surveys with HARPS and first detections Planets and brown dwarfs around A-F main-sequence stars: performances of radial-velocity surveys with HARPS and first detections

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010eas....41...99d&link_type=abstract

EAS Publications Series, Volume 41, 2010, pp.99-102

Computer Science

Performance

Scientific paper

Due to their high v sin{i}, 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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