The Discovery of a Field Methane Dwarf from Sloan Digital Sky Survey Commissioning Data

We report the discovery of the coolest field dwarf yet known, selected as an unresolved object with extremely red colors from commissioning imaging data of the Sloan Digital Sky Survey. Its spectrum from 0.8 to 2.5 μm is dominated by strong bands of H2O and CH4. Its spectrum and colors over this range are very similar to those of Gl 229B, the only other known example of a methane dwarf. It is roughly 1.2 mag fainter than Gl 229B, suggesting that it lies at a distance of ~10 pc. Such a cool object must have a mass well below the hydrogen-burning limit of 0.08 M☉ and therefore is a genuine brown dwarf, with a probable mass in the range 0.015-0.06 M☉ for an age range of 0.3-5 Gyr.

[1]  A. Burrows,et al.  Chemical Equilibrium Abundances in Brown Dwarf and Extrasolar Giant Planet Atmospheres , 1999 .

[2]  David A. Golimowski,et al.  A coronagraphic search for brown dwarfs around nearby stars , 1994 .

[3]  C. Burrows,et al.  Wide Field Planetary Camera 2 Observations of the Brown Dwarf Gliese 229B: Optical Colors and Orbital Motion , 1998 .

[4]  S. Kulkarni,et al.  Discovery of a cool brown dwarf , 1995, Nature.

[5]  Robert Lupton,et al.  A Modified Magnitude System that Produces Well-Behaved Magnitudes, Colors, and Errors Even for Low Signal-to-Noise Ratio Measurements , 1999, astro-ph/9903081.

[6]  et al,et al.  The Sloan Digital Sky Survey Photometric Camera , 1998, astro-ph/9809085.

[7]  Xiaohui Fan Simulation of Stellar Objects in SDSS Color Space , 1999 .

[8]  R. Stone Astrometric Calibration Regions Along the Celestial Equator , 1997 .

[9]  David G. Monet,et al.  Dwarfs Cooler than “M”: The Definition of Spectral Type “L” Using Discoveries from the 2-Micron All-Sky Survey (2MASS) , 1999 .

[10]  F. Allard,et al.  Synthetic Spectra and Mass Determination of the Brown Dwarf Gliese 229B , 1996 .

[11]  M. Fukugita,et al.  The Sloan Digital Sky Survey Photometric System , 1996 .

[12]  S. R. Kulkarni,et al.  The Spectrum of the Brown Dwarf Gliese 229B , 1997 .

[13]  J. B. Oke,et al.  Secondary standard stars for absolute spectrophotometry , 1983 .

[14]  T. Guillot,et al.  Atmospheric, Evolutionary, and Spectral Models of the Brown Dwarf Gliese 229 B , 1996, Science.

[15]  D. Stevenson The Search for Brown Dwarfs , 1991 .

[16]  K. Lodders,et al.  Atmospheric Chemistry of the Brown Dwarf Gliese 229B: Thermochemical Equilibrium Predictions , 1996 .

[17]  B. Oppenheimer,et al.  Infrared Spectrum of the Cool Brown Dwarf Gl 229B , 1995, Science.

[18]  A. Burrows,et al.  The science of brown dwarfs , 1993 .

[19]  S. Maddox,et al.  Wide Field Spectroscopy and the Distant Universe: The 35th Herstmonceux Conference Cambridge, United Kingdom July 4-8, 1994 , 1995 .

[20]  M. Marley,et al.  Detection of Abundant Carbon Monoxide in the Brown Dwarf Gliese 229B , 1997 .

[21]  The Near-Infrared Spectrum of the Brown Dwarf Gliese 229B , 1996, astro-ph/9606056.

[22]  Ben R. Oppenheimer,et al.  SPECTRAL ENERGY DISTRIBUTION AND BOLOMETRIC LUMINOSITY OF THE COOL BROWN DWARF GLIESE 229B , 1996 .

[23]  T. Guillot,et al.  A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs , 1997, astro-ph/9705201.

[24]  S. Leggett Infrared Colors of Low-Mass Stars , 1992 .

[25]  R. Paul Butler,et al.  DETECTION OF EXTRASOLAR GIANT PLANETS , 1998 .

[26]  David J. Robertson,et al.  Advanced cooled grating spectrometer for the UKIRT , 1990, Astronomical Telescopes and Instrumentation.

[27]  R. H. Brown,et al.  Revised Fluxes for Gliese 229B , 1999, astro-ph/9903422.

[28]  Maria Teresa Ruiz,et al.  Kelu-1 : A Free-floating Brown Dwarf in the Solar Neighborhood , 1997 .