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...
Main Authors: | , , , , , , , , |
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Other Authors: | |
Language: | en |
Published: |
EDP SCIENCES S A
2017
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Subjects: | |
Online Access: | http://hdl.handle.net/10150/625997 http://arizona.openrepository.com/arizona/handle/10150/625997 |