SpeX Spectroscopy of Unresolved Very Low Mass Binaries. II. Identification of Fourteen Candidate Binaries with Late-M/Early-L and T Dwarf Components

1 code implementation • 13 Aug 2014 • Daniella C. Bardalez Gagliuffi, Adam J. Burgasser, Christopher R. Gelino, Dagny L. Looper, Christine P. Nicholls, Sarah J. Schmidt, Kelle Cruz, Andrew A. West, John E. Gizis, Stanimir Metchev

Multiplicity is a key statistic for understanding the formation of very low mass (VLM) stars and brown dwarfs.

Solar and Stellar Astrophysics