Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes

Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes

Context. One of the key questions of the star formation problem is whether brown dwarfs (BDs) form in the manner of stars directly from the gravitational collapse of a molecular cloud core (star-like) or whether BDs and some very low-mass stars (VLMSs) constitute a separate population that forms alo...

Full description

Bibliographic Details
Main Authors: Marks, M., Martín, E. L., Béjar, V. J. S., Lodieu, N., Kroupa, P., Manjavacas, E., Thies, I., Rebolo López, R., Velasco, S.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: EDP SCIENCES S A 2017
Subjects:
binaries: general
stars: late-type
stars: low-mass
brown dwarfs
stars: formation
Online Access:http://hdl.handle.net/10150/625997
http://arizona.openrepository.com/arizona/handle/10150/625997

Internet

http://hdl.handle.net/10150/625997
http://arizona.openrepository.com/arizona/handle/10150/625997

Similar Items