{ "id": "0903.3219", "version": "v2", "published": "2009-03-18T18:41:03.000Z", "updated": "2009-03-28T07:42:52.000Z", "title": "PHL 5038: A spatially resolved white dwarf + brown dwarf binary", "authors": [ "P. R. Steele", "M. R. Burleigh", "J. Farihi", "B. T. Gaensicke", "R. F. Jameson", "P. D. Dobbie", "M. A. Barstow" ], "comment": "5 pages, 3 figures, accepted to A&A", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "A near-infrared excess is detected at the white dwarf PHL5038 in UKIDSS photometry, consistent with the presence of a cool, substellar companion. We have obtained H- and K-grism spectra and images of PHL5038 using NIRI on Gemini North. The target is spatially and spectrally resolved into two components; an 8000K 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 55AU, and so it becomes only the second known wide WD+dL binary to be found after GD165AB. This object could potentially be used as a benchmark for testing substellar evolutionary models at intermediate to older ages.", "revisions": [ { "version": "v2", "updated": "2009-03-28T07:42:52.000Z" } ], "analyses": { "keywords": [ "spatially resolved white dwarf", "brown dwarf binary", "8000k da white dwarf", "l8 brown dwarf companion", "testing substellar evolutionary models" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/200911694", "journal": "Astronomy and Astrophysics", "year": 2009, "month": "Jun", "volume": 500, "number": 3, "pages": 1207 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 815753, "adsabs": "2009A&A...500.1207S" } } }