Discovery of Two Very Low-Mass Binaries: Final Results of an Adaptive Optics Survey of Nearby M6.0-M7.5 Stars

Details Discovery of Two Very Low-Mass Binaries: Final Results of an Adaptive Optics Survey of Nearby M6.0-M7.5 Stars Discovery of Two Very Low-Mass Binaries: Final Results of an Adaptive Optics Survey of Nearby M6.0-M7.5 Stars

2004-12-10

arxiv.org/abs/astro-ph/0412240v1

Astrophys.J. 621 (2005) 1023-1032

Astronomy and Astrophysics

Astrophysics

20 pages, 8 figures, accepted to ApJ

Scientific paper

10.1086/427743

We present updated results of a high-resolution, magnitude limited (Ks<12 mag) imaging survey of nearby low-mass M6.0-M7.5 field stars. The observations were carried out using adaptive optics at the Gemini North, VLT, Keck II, and Subaru telescopes. Our sample of 36 stars consists predominantly of nearby (<30 pc) field stars, 5 of which we have resolved as binaries. Two of the binary systems, 2MASSI J0429184-312356 and 2MASSI J1847034+552243, are presented here for the first time. All 5 discovered binary systems have separations between 0.08"-0.53" (2-9 AU) with similar mass ratios (q>0.8, delta Ks < 1 mag). This result supports the hypothesis that wide (a>20 AU) very low-mass (M_tot<0.19 M_sun) binary systems are rare. The projected semimajor axis distribution of these systems peak at ~ 5 AU and we report a sensitivity-corrected binary fraction of 9% (-3%, +4%) for stars with primaries of spectral type M6.0-M7.5 with separations >3 AU and mass ratios q>0.6. Within these instrumental sensitivities, these results support the overall trend that both the semimajor axis distribution and binary fraction are a function of the mass of the primary star and decrease with decreasing primary mass. These observations provide important constraints for low-mass binary star formation theories.

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