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The Carina-Near Moving Group

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Zuckerman, B; Bessell, Michael; Song, Inseok; Kim, S

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We identify a group of ∼20 comoving, mostly southern hemisphere, ∼200 Myr old stars near Earth. Of the stars likely to be members of this Carina-Near moving group, in either its nucleus (∼30 pc from Earth) or its surrounding stream, all but three ar

dc.contributor.authorZuckerman, B
dc.contributor.authorBessell, Michael
dc.contributor.authorSong, Inseok
dc.contributor.authorKim, S
dc.date.accessioned2015-12-08T22:16:12Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/30568
dc.description.abstractWe identify a group of ∼20 comoving, mostly southern hemisphere, ∼200 Myr old stars near Earth. Of the stars likely to be members of this Carina-Near moving group, in either its nucleus (∼30 pc from Earth) or its surrounding stream, all but three ar
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Open clusters and associations: individual (HR 3070 moving group); Stars: evolution; Stars: kinematics; Stars: pre-main-sequence
dc.titleThe Carina-Near Moving Group
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume649
dc.date.issued2006
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4114753xPUB75
local.type.statusPublished Version
local.contributor.affiliationZuckerman, B, University of California
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSong, Inseok, Gemini Observatory
local.contributor.affiliationKim, S, Gemini Observatory
local.description.embargo2037-12-31
local.bibliographicCitation.startpageL115
local.bibliographicCitation.lastpageL118
local.identifier.doi10.1086/508060
dc.date.updated2015-12-08T07:58:34Z
local.identifier.scopusID2-s2.0-33751409188
CollectionsANU Research Publications

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