ULAS J141623.94134836.3 - a faint common proper motion companion of a nearby L dwarf. Serendipitous discovery of a cool brown dwarf in UKIDSS DR6
arXiv:1001.2743 · doi:10.1051/0004-6361/201014078
Abstract
New near-infrared large-area sky surveys (e.g. UKIDSS, CFBDS, WISE) go deeper than 2MASS and aim at detecting brown dwarfs lurking in the Solar neighbourhood which are even fainter than the latest known T-type objects, so-called Y dwarfs. Using UKIDSS data, we have found a faint brown dwarf candidate with very red optical-to-near-infrared but extremely blue near-infrared colours next to the recently discovered nearby L dwarf SDSS J141624.08134826.7. We check if the two objects are co-moving by studying their parallactic and proper motion and compare the new object with known T dwarfs. The astrometric measurements are consistent with a physical pair (75 AU) at a distance 8 pc. The extreme colour (1.7) and absolute magnitude (=17.780.46 and =19.450.52) make the new object appear as one of the coolest (T600 K) and nearest brown dwarfs, probably of late-T spectral type and possibly with a high surface gravity (log 5.0).
accepted for publication as a Letter in Astronomy and Astrophysics, 4 pages, 7 figures, changed subtitle and discussion, former Fig. 4 removed, new Figs. 2, 6, and 7
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