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A new method to identify nearby, young, low-mass stars

Rodriguez, David R.; Bessell, Michael; Zuckerman, B.; Kastner, Joel H.

Description

We describe a new method to identify young, late-type stars within ∼150 pc of the Earth that employs visual or near-infrared (NIR) data and the GALEX GR4/5 database. For spectral types later than K5, we demonstrate that the ratio of GALEX near-ultraviol

dc.contributor.authorRodriguez, David R.
dc.contributor.authorBessell, Michael
dc.contributor.authorZuckerman, B.
dc.contributor.authorKastner, Joel H.
dc.date.accessioned2015-12-10T23:16:11Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/64955
dc.description.abstractWe describe a new method to identify young, late-type stars within ∼150 pc of the Earth that employs visual or near-infrared (NIR) data and the GALEX GR4/5 database. For spectral types later than K5, we demonstrate that the ratio of GALEX near-ultraviol
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyright
dc.sourceAstrophysical Journal, The
dc.titleA new method to identify nearby, young, low-mass stars
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume727
dc.date.issued2011
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationf2965xPUB1028
local.type.statusPublished Version
local.contributor.affiliationRodriguez, David R., University of California
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationZuckerman, B., University of California
local.contributor.affiliationKastner, Joel H., Rochester Institute of Technology
local.bibliographicCitation.issue2
local.bibliographicCitation.startpage1
local.bibliographicCitation.lastpage10
local.identifier.doi10.1088/0004-637X/727/2/62
dc.date.updated2015-12-10T09:50:37Z
local.identifier.scopusID2-s2.0-84891214544
local.identifier.thomsonID000286662000001
dcterms.accessRightsOpen Access
CollectionsANU Research Publications

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