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Discovery of Four Field Methane (T-Type) Dwarfs with the Two Micron All-Sky Survey
Author(s) -
Adam J. Burgasser,
J. Davy Kirkpatrick,
Michael E. Brown,
I. Neill Reid,
John E. Gizis,
C. C. Dahn,
D. G. Monet,
Charles Beichman,
James Liebert,
R. M. Cutri,
Michael F. Skrutskie
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/312221
Subject(s) - physics , brown dwarf , sky , astrophysics , stellar classification , astronomy , stars
We report the discovery of four field methane ("T"-type) brown dwarfs using Two Micron All-Sky Survey (2MASS) data. One additional methane dwarf, previously discovered by the Sloan Digital Sky Survey, was also identified. Near-infrared spectra clearly show the 1.6 and 2.2 µm CH4 absorption bands characteristic of objects with Teff < 1300 K, as well as broadened H2O bands at 1.4 and 1.9 µm. Comparing the spectra of these objects with that of Gl 229B, we propose that all new 2MASS T dwarfs are warmer than 950 K, in order from warmest to coolest: 2MASS J1217-03, J1225-27, J1047+21 and J1237+65. Based on this preliminary sample, we find a warm T dwarf surface density of 0.0022 T dwarfs/sq. deg., or 90 warm T dwarfs over the whole sky detectable to J < 16. The resulting space density upper limit, 0.01 T dwarfs/pc3, is

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