The M dwarf planet search program with the VLT+UVES

Details The M dwarf planet search program with the VLT+UVES The M dwarf planet search program with the VLT+UVES

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..457k&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

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Low Luminosity Stars, Subdwarfs, And Brown Dwarfs, Extrasolar Planetary Systems, Star Formation

Scientific paper

We present results from our precision radial velocity survey of M dwarfs with the VLT+UVES in search for planetary companions. They include the first genuine brown dwarf desert object and several low-mass companion candidates around early-type M dwarfs. The lack of Jupiter-mass companions in this survey is compared with results from other search programs. Upper limits to the mass of hypo-thetical planets can be placed down to the Earth mass regime in the habitable zones of our better observed stars.

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