2MASS J22521073-1730134: A Resolved L/T Binary at 14 Parsecs

Details 2MASS J22521073-1730134: A Resolved L/T Binary at 14 Parsecs 2MASS J22521073-1730134: A Resolved L/T Binary at 14 Parsecs

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006apj...639.1114r&link_type=abstract

The Astrophysical Journal, Volume 639, Issue 2, pp. 1114-1119.

Astronomy and Astrophysics

Astronomy

26

Stars: Binaries: Visual, Stars: Individual (2Massw J22521073-1730134), Stars: Low-Mass, Brown Dwarfs

Scientific paper

NICMOS images of the nearby late-type L dwarf 2MASS J22521073-1730134 (DENIS-P J225210.73-173013.4) show that it is a close double, separation 0.13". The companion is 1.0 mag fainter than the primary in the F110W passband and 1.55 mag fainter in the F170M images. The latter passband is centered on the 1.6 μm methane band. The small separation and the absence of an optical counterpart suggest that the two sources are associated; the relatively blue infrared color suggests that 2MASS J22521073-1730134B is a T-type binary companion of the late-L primary. This hypothesis is supported by infrared spectroscopy, which shows weak methane absorption in both the H and K passbands. We estimate a distance of 13.6+3.8-2.6 pc to the system and a projected linear separation of 1.75 AU. We consider the potential for measuring dynamical masses of the two components.
Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.

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