L-Dwarf Binaries in the 20-Parsec Sample

Details L-Dwarf Binaries in the 20-Parsec Sample L-Dwarf Binaries in the 20-Parsec Sample

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aj....135..580r&link_type=abstract

The Astronomical Journal, Volume 135, Issue 2, pp. 580-587 (2008).

Astronomy and Astrophysics

Astronomy

12

Binaries: Visual, Stars: Low-Mass, Brown Dwarfs

Scientific paper

We have used the NICMOS NIC1 camera on the Hubble Space Telescope to obtain high-resolution near-infrared images of 27 nearby ultracool dwarfs with formal distance estimates less than 20 parsecs. One target, 2MASS J22551861-5713056, is resolved as a binary system, with a 4:1 flux ratio in the F110W passband. The primary has spectral type L6, and the revised spectroscopic parallax places it at a distance of ~12 parsecs. The secondary is likely to have a spectral type between L8 and T1. The remaining 26 dwarfs are unresolved. Combining the present results with our earlier NICMOS (Near-Infrared Camera and Multi Object Spectrometer) observations and literature data, high-resolution imaging exists for 72 of the 85 L dwarfs in the current 20-parsec census. We derive a formal frequency of 15.3+5.1 -3.3% for resolved binaries in the local L-dwarf population. The frequency drops to 12.5+5.3 -3.0% if we take Malmquist bias into account. The NICMOS observations are capable of detecting systems with mass ratios q>0.2, but all known binaries are near equal-mass, suggesting that low-q systems either fail to form, or have short lifetimes.
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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