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A 2MASS L Dwarf Companion to the Nearby K Dwarf GJ 1048
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to appear in April 2001 Astronomical Journal
A 2MASS L Dwarf Companion to the Nearby K Dwarf GJ 1048
John E. Gizis1, J. Davy Kirkpatrick
Infrared Processing and Analysis Center, 100-22, California Institute of Technology, Pasadena,
CA 91125
gizis@,davy@
John C. Wilson
Space Sciences, Cornell University, Ithaca, NY 14853
jcw14@
ABSTRACT
We report the discovery of a probable L1 companion to the nearby K2 dwarf GJ 1048
using the Two Micron All-Sky Survey (2MASS). This source, 2MASSI J0235599-233120
or GJ 1048B, has 2MASS near-infrared colors and absolute magnitudes consistent with
an early L dwarf companion with a projected separation of 250 A.U. The L1 spectral
type is confirmed by far-red optical and low-resolution IR spectroscopy. We present
evidence that GJ 1048 is a young (. 1Gyr) system, and that GJ 1048B may be a high-
mass brown dwarf below the hydrogen-burning limit. Additional studies of the GJ 1048
system will help constrain the characteristics of L dwarfs as a function of age and mass.
Subject headings: binaries: general — solar neighborhood — stars: low-mass, brown
dwarfs
1. Introduction
Brown dwarfs are very-low-mass dwarfs which are unable to maintain a stable luminosity
by hydrogen fusion. Analysis of radial velocity surveys has identified a “brown dwarf desert” —
although stellar and planetary companions to FGKM main sequence stars are relatively common,
less than 1% of such stars have companions in the range 0.005 - 0.08 M⊙ within 3 A.U.(Mazeh et al.
1Visiting Astronomer, Kitt Peak National Observatory, National Optical Astronomy Observatories, which is op-
erated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with
the National Science Foundation.
– 2 –
1992; Marcy Butler 2000). Although brown dwarfs are rare as short-period companions to more
massive stars, they are quite common in the field. The Deep Near-Infrared Survey (DE
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