A companion to AB Pic at the planet/brown dwarf boundary

G. Chauvin*, A. M. Lagrange, B. Zuckerman, C. Dumas, D. Mouillet, I. Song, J. L. Beuzit, P. Lowrance, M. S. Bessell

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    218 Citations (Scopus)

    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 languageEnglish
    Pages (from-to)L29-L32
    JournalAstronomy and Astrophysics
    Volume438
    Issue number3
    DOIs
    Publication statusPublished - Aug 2005

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