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New members of the Scorpius-Centaurus complex and ages of its sub-regions

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dc.contributor.authorSong, Inseok
dc.contributor.authorZuckerman, B
dc.contributor.authorBessell, Michael
dc.date.accessioned2015-12-10T23:15:55Z
dc.date.issued2012
dc.date.updated2016-02-24T08:35:01Z
dc.description.abstractWe have spectroscopically identified ∼100 G-, K-, and M-type members of the Scorpius-Centaurus complex. To deduce the age of these young stars we compare their Liλ6708 absorption line strengths against those of stars in the TW Hydrae association and β
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/64846
dc.publisherUniversity of Chicago Press
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstronomical Journal
dc.subjectKeywords: open clusters and associations: individual (Scorpius OB2, Lower Centaurus-Crux, Upper Centaurus-Lupus, Upper Scorpius); stars: activity; stars: kinematics and dynamics; stars: pre-main sequence
dc.titleNew members of the Scorpius-Centaurus complex and ages of its sub-regions
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.contributor.affiliationSong, Inseok, University of Georgia
local.contributor.affiliationZuckerman, B, University of California
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidBessell, Michael, u6900904
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB1008
local.identifier.citationvolume144
local.identifier.doi10.1088/0004-6256/144/1/8
local.identifier.scopusID2-s2.0-84862553580
local.identifier.thomsonID000305418600008
local.type.statusPublished Version

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