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The discovery of the T8.5 dwarf UGPS J0521+3640

Identifieur interne : 006307 ( Main/Exploration ); précédent : 006306; suivant : 006308

The discovery of the T8.5 dwarf UGPS J0521+3640

Auteurs : Ben Burningham [Royaume-Uni] ; P. W. Lucas ; S. K. Leggett [États-Unis] ; R. Smart [Italie] ; D. Baker ; D. J. Pinfield ; C. G. Tinney [Australie] ; D. Homeier [Allemagne] ; F. Allard [France] ; Z. H. Zhang ; J. Gomes ; A. C. Day-Jones [Chili] ; H. R. A. Jones ; G. Kovács ; N. Lodieu [Espagne] ; F. Marocco ; D. N. Murray ; B. Sip Cz

Source :

RBID : ISTEX:626E1834DFAB73F5E26BD0EB949F46A3F4F91909

English descriptors

Abstract

We have carried out a search for late‐type T dwarfs in the UKIRT Infrared Deep Sky Survey Galactic Plane Survey 6th Data Release. The search yielded two persuasive candidates, both of which have been confirmed as T dwarfs. The brightest, UGPS J0521+3640, has been assigned the spectral type T8.5 and appears to lie at a distance of 7–9 pc. The fainter of the two, UGPS J0652+0324, is classified as a T5.5 dwarf and lies at an estimated distance of 28–37 pc. Warm‐Spitzer observations in IRAC channels 1 and 2, taken as part of the GLIMPSE360 Legacy Survey, are available for UGPS J0521+3640 and we used these data with the near‐infrared spectroscopy to estimate its properties. We find best‐fitting solar metallicity BT‐Settl models for Teff= 600 and 650 K and log g= 4.5 and 5.0. These parameters suggest a mass between 14 and 32MJ for an age between 1 and 5 Gyr. The proximity of this very cool T dwarf, and its location in the Galactic plane, makes it an ideal candidate for high‐resolution adaptive optics imaging to search for cool companions.

Url:
DOI: 10.1111/j.1745-3933.2011.01062.x


Affiliations:


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<div type="abstract" xml:lang="en">We have carried out a search for late‐type T dwarfs in the UKIRT Infrared Deep Sky Survey Galactic Plane Survey 6th Data Release. The search yielded two persuasive candidates, both of which have been confirmed as T dwarfs. The brightest, UGPS J0521+3640, has been assigned the spectral type T8.5 and appears to lie at a distance of 7–9 pc. The fainter of the two, UGPS J0652+0324, is classified as a T5.5 dwarf and lies at an estimated distance of 28–37 pc. Warm‐Spitzer observations in IRAC channels 1 and 2, taken as part of the GLIMPSE360 Legacy Survey, are available for UGPS J0521+3640 and we used these data with the near‐infrared spectroscopy to estimate its properties. We find best‐fitting solar metallicity BT‐Settl models for Teff= 600 and 650 K and log g= 4.5 and 5.0. These parameters suggest a mass between 14 and 32MJ for an age between 1 and 5 Gyr. The proximity of this very cool T dwarf, and its location in the Galactic plane, makes it an ideal candidate for high‐resolution adaptive optics imaging to search for cool companions.</div>
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