Issue |
A&A
Volume 440, Number 2, September III 2005
|
|
---|---|---|
Page(s) | L55 - L58 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:200500167 | |
Published online | 01 September 2005 |
Letter to the Editor
The first wide ultracool binary dwarf in the field: DENIS-J055146.0-443412.2 (M8.5 + L0)
1
European Southern Observatory, Casilla 19001, Santiago 19, Chile e-mail: mbillere@eso.org
2
Laboratoire d'Astrophysique de Grenoble, Observatoire de Grenoble, BP 53, 38041 Grenoble, France
3
Canada-France-Hawaii Telescope Corporation, 65-1238 Mamaloha Highway, Kamuela, HI 96743, USA
4
Instituto de Astrofísica de Canarias, 38200 La Laguna, Spain
Received:
18
July
2005
Accepted:
29
July
2005
We present observations of a new very low mass field binary, discovered during an infrared imaging survey of 250 DENIS L and very late-M dwarfs. DENIS-J055146.0-443412.2 is an M8.5 + L0 pair, with a physical separation of over 200 AU. This makes it the widest very low mass binary known in the field, by an order of magnitude. Such a system is fragile, and it would not have survived a close encounter with a third body. Its existence demonstrate that some very low mass stars/brown dwarfs form without ejection from a multiple system, or any other strong dynamical interaction.
Key words: stars / brown dwarfs / binary system / formation
© ESO, 2005
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