Discovery of the Widest Very Low Mass Binary
Author(s) -
Étienne Artigau,
David Lafrenière,
René Doyon,
Loïc Albert,
Daniel Nadeau,
Jasmin Robert
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/516710
Subject(s) - binary number , binary system , mass spectrum , physics , astrophysics , low mass , component (thermodynamics) , spectral line , mass ratio , mass spectrometry , astronomy , mathematics , stars , thermodynamics , arithmetic , quantum mechanics
We report the discovery of a very low mass binary system (primary mass <0.1Msol) with a projected separation of ~5100 AU, more than twice that of thewidest previously known system. A spectrum covering the 1-2.5 micronswavelength interval at R ~1700 is presented for each component. Analysis of thespectra indicates spectral types of M6.5V and M8V, and the photometric distanceof the system is ~62 pc. Given that previous studies have established that nomore than 1% of very low mass binary systems have orbits larger than 20 AU, theexistence of such a wide system has a bearing on very low mass star formationand evolution models.Comment: accepted ApJL, 4 page
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