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PHL 5038: A spatially resolved white dwarf + brown dwarf binary

Steele, PR; Burleigh, MR; Farihi, J; Gänsicke, BT; Jameson, RF; Dobbie, PD; Barstow, MA; (2009) PHL 5038: A spatially resolved white dwarf + brown dwarf binary. Astronomy and Astrophysics , 500 (3) pp. 1207-1210. 10.1051/0004-6361/200911694. Green open access

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Abstract

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 0.94″. 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.

Type: Article
Title: PHL 5038: A spatially resolved white dwarf + brown dwarf binary
Open access status: An open access version is available from UCL Discovery
DOI: 10.1051/0004-6361/200911694
Publisher version: http://dx.doi.org/10.1051/0004-6361/200911694
Language: English
Additional information: Reproduced with permission from Astronomy & Astrophysics, © ESO.
Keywords: white dwarfs -- stars: low-mass, brown dwarfs -- binaries: general -- binaries: visual
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/1477420
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