Issue |
A&A
Volume 425, Number 2, October II 2004
|
|
---|---|---|
Page(s) | L29 - L32 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:200400056 | |
Published online | 21 September 2004 |
Letter to the Editor
A giant planet candidate near a young brown dwarf*
Direct VLT/NACO observations using IR wavefront sensing
1
European Southern Observatory, Casilla 19001, Santiago 19, Chile e-mail: gchauvin@eso.org
2
Laboratoire d'Astrophysique, Observatoire de Grenoble, 414 rue de la piscine, Saint-Martin d'Hères, France
3
Department of Physics & Astronomy and Center for Astrobiology, University of California, Los Angeles, 8371 Math Science Building, Box 951562, CA 90095-1562, USA
4
Laboratoire d'Astrophysique, Observatoire Midi-Pyrénées, Tarbes, France
5
Spitzer Science Center, Infrared Processing and Analysis Center, MS 220-6, Pasadena, CA 91125, USA
Received:
22
July
2004
Accepted:
12
August
2004
We present deep VLT/NACO infrared imaging and spectroscopic observations of the brown dwarf 2MASSWJ 1207334-393254, obtained during our on-going adaptive optics survey of southern young, nearby associations. This ~25 brown dwarf, located ~70 pc from Earth, has been recently identified as a member of the TW Hydrae Association (age ~ 8 Myr). Using adaptive optics infrared wavefront sensing to acquire sharp images of its circumstellar environment, we discovered a very faint and very red object at a close separation of ~780 mas (~55 AU). Photometry in the H,
and
bands and upper limit in J-band are compatible with a spectral type L5-L9.5. Near-infrared spectroscopy is consistent with this spectral type estimate. Different evolutionary models predict an object within the planetary regime with a mass of
and an effective temperature of
K.
Key words: 2MASSWJ 1207334-393254 / brown dwarf / giant planet / adaptive optics imaging and spectroscopy
© ESO, 2004
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