The Multiplicity of M Dwarfs in Young Moving Groups

The Multiplicity of M Dwarfs in Young Moving Groups

We image 104 newly identified low-mass (mostly M-dwarf) pre-main sequence (PMS) members of nearby young moving groups (YMGs) with Magellan Adaptive Optics (MagAO) and identify 27 stellar binaries with instantaneous projected separation as small as 40 mas. Fifteen were previously unknown. The total n...

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Bibliographic Details
Main Authors: Shan, Yutong, Yee, Jennifer C., Bowler, Brendan P., Cieza, Lucas A., Montet, Benjamin T., Cánovas, Héctor, Liu, Michael C., Close, Laird M., Hinz, Phil M., Males, Jared R., Morzinski, Katie M., Vaz, Amali, Bailey, Vanessa P., Follette, Katherine B.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
binaries: visual
methods: observational
methods: statistical
stars: low-mass
stars: pre-main sequence
techniques: photometric
Online Access:http://hdl.handle.net/10150/627110
http://arizona.openrepository.com/arizona/handle/10150/627110

Internet

http://hdl.handle.net/10150/627110
http://arizona.openrepository.com/arizona/handle/10150/627110

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