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18 April 2024
 
  » arxiv » 1211.6977

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Parallaxes and Proper Motions of Ultracool Brown Dwarfs of Spectral Types Y and Late T
Kenneth A. Marsh ; Edward L. Wright ; J. Davy Kirkpatrick ; Christopher R. Gelino ; Michael C. Cushing ; Roger L. Griffith ; Michael F. Skrutskie ; Peter R. Eisenhardt ;
Date 29 Nov 2012
AbstractWe present astrometric measurements of eleven nearby ultracool brown dwarfs of spectral types Y and late-T, based on imaging observations from a variety of space-based and ground-based telescopes. These measurements have been used to estimate relative parallaxes and proper motions via maximum likelihood fitting of geometric model curves. To compensate for the modest statistical significance (<~ 7) of our parallax measurements we have employed a novel Bayesian procedure for distance estimation which makes use of an a priori distribution of tangential velocities, Vtan, assumed similar to that implied by previous observations of T dwarfs. Our estimated distances are therefore somewhat dependent on that assumption. Nevertheless, the results have yielded distances for five of our eight Y dwarfs and all three T dwarfs. Estimated distances in all cases are >~ 3 pc. In addition, we have obtained significant estimates of Vtan for two of the Y dwarfs; both are <100 km/s, consistent with membership in the thin disk population. Comparison of absolute magnitudes with model predictions as a function of color shows that the Y dwarfs are significantly redder in J-H than predicted by a cloud-free model
Source arXiv, 1211.6977
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