Abstract
We report deep imaging observations of the young, nearby star AB Pic, a member of the large Tucana-Horologium association. We have detected a faint, red source 5.5″ South of the star with JHK colors compatible with that of a young substellar L dwarf. Follow-up observations at two additional epochs confirm, with a confidence level of 4.7σ, that the faint red object is a companion to AB Pic rather than it being a stationary background object. A low resolution K-band spectrum indicates an early-L spectral type for the companion. Finally, evolutionary model predictions based on the JHK photometry of AB Pic b indicate a mass of 13 to 14 MJup if its age is ∼30 Myr. Is AB Pic b a massive planet or a minimum mass brown dwarf?
Original language | English |
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Pages (from-to) | L29-L32 |
Journal | Astronomy and Astrophysics |
Volume | 438 |
Issue number | 3 |
DOIs | |
Publication status | Published - Aug 2005 |