Volume 500, Number 3, June IV 2009
|Page(s)||1207 - 1210|
|Section||Stellar structure and evolution|
|Published online||08 April 2009|
PHL 5038: a spatially resolved white dwarf brown dwarf binary
Department of Physics & Astronomy, University of Leicester, Leicester, LE1 7RH, UK e-mail: email@example.com
2 Department of Physics, University of Warwick, Coventry, CV4 7AL, UK
3 Anglo-Australian Observatory, PO Box 296, Epping, Sydney, NSW 1710, Australia
Accepted: 19 March 2009
A near-infrared excess is detected at the white dwarf PHL 5038 in UKIDSS photometry, consistent with the presence of a cool, substellar companion. We have obtained H- and K-grism spectra and images of PHL 5038 using NIRI on Gemini North. The target is spatially and spectrally resolved into two components: an 8000 K DA white dwarf, and a likely L8 brown dwarf companion, separated by . The spectral type of the secondary was determined using standard spectral indices for late L and T dwarfs. The projected orbital separation of the binary is 55 AU, so it becomes only the second known wide WD+dL binary to be found after GD 165AB. This object could potentially be used as a benchmark for testing substellar evolutionary models at intermediate to older ages.
Key words: white dwarfs / stars: low-mass, brown dwarfs / binaries: general / binaries: visual
© ESO, 2009
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