Planck-dust-allsky

Discovery of Three Distant, Cold Brown Dwarfs in the WFC3 Infrared Spectroscopic Parallels Survey

June 2012 • 2012ApJ...752L..14M

Authors • Masters, D. • McCarthy, P. • Burgasser, A. J. • Hathi, N. P. • Malkan, M. • Ross, N. R. • Siana, B. • Scarlata, C. • Henry, A. • Colbert, J. • Atek, H. • Rafelski, M. • Teplitz, H. • Bunker, A. • Dressler, A.

Abstract • We present the discovery of three late-type (>=T4.5) brown dwarfs, including a probable Y dwarf, in the WFC3 Infrared Spectroscopic Parallels (WISP) survey. We use the G141 grism spectra to determine the spectral types of the dwarfs and derive distance estimates based on a comparison with nearby T dwarfs with known parallaxes. These are the most distant spectroscopically confirmed T/Y dwarfs, with the farthest at an estimated distance of ~400 pc. We compare the number of cold dwarfs found in the WISP survey with simulations of the brown dwarf mass function. The number found is generally consistent with an initial stellar mass function dN/dMvpropM with α = 0.0-0.5, although the identification of a Y dwarf is somewhat surprising and may be indicative of either a flatter absolute magnitude/spectral-type relation than previously reported or an upturn in the number of very-late-type brown dwarfs in the observed volume.

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IPAC Authors
(alphabetical)

James Colbert

Associate Scientist


Elise_furlan

Elise Furlan

Associate Scientist


Daniel Masters

Assistant Scientist


Harry_teplitz

Harry Teplitz

Senior Scientist