4.7 Article

Southern very low mass stars and brown dwarfs in wide binary and multiple systems

Journal

ASTROPHYSICAL JOURNAL
Volume 667, Issue 1, Pages 520-526

Publisher

IOP PUBLISHING LTD
DOI: 10.1086/520873

Keywords

binaries : visual; stars : formation; stars : individual (2MASS J23310161-0406193 AB, HD 221356, LP 655-23); stars : low-mass, brown dwarfs

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The results of the Konigstuhl survey in the Southern Hemisphere are presented. I have searched for common proper motion companions to 173 field very low mass stars and brown dwarfs with spectral types > M5.0 V and magnitudes J less than or similar to 14.5 mag. I have measured for the first time the common proper motion of two new wide systems containing very low mass components, Konigstuhl 2 AB and 3 A-BC. Together with Konigstuhl 1 AB and 2M 0126-50 AB, they are among the widest systems in their respective classes (r = 450-11,900 AU). I have determined the minimum frequency of field wide multiples (r > 100 AU) with late-type components at 5.0% +/- 0.9% and the frequency of field wide late-type binaries with mass ratios q > 0.5 at 1.2% +/- 0: 9%. These values represent a key diagnostic of evolution history and low-mass star and brown dwarf formation scenarios. In addition, the proper motions of 62 field very low mass dwarfs are measured here for the first time.

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