Identification of a Wide, Low-Mass Multiple System Containing the Brown Dwarf 2MASS J0850359+105716
Jacqueline K. Faherty, Adam J. Burgasser, John J. Bochanski, Dagny L., Looper, Andrew A. West, Nicole S. van der Bliek

TL;DR
This paper reports the discovery of a wide, low-mass quadruple system including a brown dwarf and a binary M dwarf, providing insights into the formation and characteristics of such low-binding-energy systems.
Contribution
The study identifies a rare wide, low-mass quadruple system with detailed age and mass estimates, and discusses its implications for formation models of brown dwarf systems.
Findings
System is a wide, low-mass quadruple with ~7700 AU separation.
Age estimates suggest the system is between 0.25-1.5 Gyr.
System's formation aligns with gravitational fragmentation models.
Abstract
We report our discovery of NLTT 20346 as an M5+M6 companion system to the tight binary (or triple) L dwarf 2MASS J0850359+105716. This nearby (~31 pc), widely separated (~7700 AU) quadruple system was identified through a cross-match of proper motion catalogs. Follow-up imaging and spectroscopy of NLTT 20346 revealed it to be a magnetically active M5+M6 binary with components separated by ~2" (50-80 AU). Optical spectroscopy of the components show only moderate Halpha emission corresponding to a statistical age of ~5 - 7 Gyr for both M dwarfs. However NLTT 20346 is associated with the XMM-Newton source J085018.9+105644, and based on X-ray activity the age of NLTT 20346 is between 250-450 Myr. Strong Li absorption in the optical spectrum of 2MASS J0850+1057 indicates an upper age limit of 0.8 - 1.5 Gyr favoring the younger age for the primary. Using evolutionary models in combination…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Astronomy and Astrophysical Research
