Discovery of the Widest Very Low Mass Binary
Open Access
- 9 March 2007
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 659 (1), L49-L52
- https://doi.org/10.1086/516710
Abstract
We report the discovery of a very low mass binary system (primary mass <0.1 Msol) with a projected separation of ~5100 AU, more than twice that of the widest previously known system. A spectrum covering the 1-2.5 microns wavelength interval at R ~1700 is presented for each component. Analysis of the spectra indicates spectral types of M6.5V and M8V, and the photometric distance of the system is ~62 pc. Given that previous studies have established that no more than 1% of very low mass binary systems have orbits larger than 20 AU, the existence of such a wide system has a bearing on very low mass star formation and evolution modelsKeywords
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