A&A 460, L19-L22 (2006)
DOI: 10.1051/0004-6361:20066120
Letter
Five new very low mass binaries
G. Montagnier1, 2, D. Ségransan2, J.-L. Beuzit1, T. Forveille3, 1, P. Delorme1, X. Delfosse1, C. Perrier1, S. Udry2, M. Mayor2, G. Chauvin4, A.-M. Lagrange1, D. Mouillet5, T. Fusco6, P. Gigan7, and E. Stadler11 Laboratoire d'Astrophysique de Grenoble, BP 53, 38041 Grenoble Cedex, France
e-mail: Guillaume.Montagnier@obs.ujf-grenoble.fr
2 Observatoire de Genève, 51 chemin des Maillettes, 1290 Sauverny, Switzerland
3 Canada-France-Hawaii Telescope Corporation, 65-1238 Mamalahoa Highway, Kamuela, HI 96743, Hawaii, USA
4 European Southern Observatory, Casilla 19001, Santiago 19, Chile
5 Laboratoire d'Astrophysique de Toulouse et Tarbes, BP 826, 65008 Tarbes Cedex, France
6 ONERA-DOTA, BP 72, 29 avenue de la Division Leclerc, 92322 Châtillon Cedex, France
7 Laboratoire d'Études Spatiales et d'Instrumentation Astrophysique, 92195 Meudon Cedex, France
(Received 26 July 2006 / Accepted 12 October 2006)
Abstract
We report the discovery of companions to 5 nearby late M dwarfs
(>M5), LHS1901, LHS4009, LHS6167, LP869-26 and WT460, and we confirm
that the recently discovered mid-T brown dwarf companion to SCR1845-6357 is
physically bound to that star.
These discoveries result from our adaptive optics survey of all M dwarfs
within 12 pc. The new companions have spectral types M5 to L1, and
orbital separations between 1 and 10 AU. They add
significantly to the number of late M dwarfs binaries in the
immediate solar neighbourhood, and will improve the multiplicity
statistics of late M dwarfs. The expected periods range from 3 to 130
years. Several pairs thus have good potential for accurate mass
determination in this poorly sampled mass range.
Key words: binaries: visual -- stars: low-mass, brown dwarfs -- techniques: high angular resolution -- instrumentation: adaptive optics
© ESO 2006

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