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The AB Doradus Moving Group

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dc.contributor.authorZuckerman, B
dc.contributor.authorSong, Inseok
dc.contributor.authorBessell, Michael
dc.date.accessioned2015-12-13T23:11:21Z
dc.date.available2015-12-13T23:11:21Z
dc.date.issued2004
dc.date.updated2016-02-24T09:48:09Z
dc.description.abstractFrom radio to X-ray wavelengths, AB Doradus has been an intensively studied star. We have identified ∼30 nearby star systems, each with one or more characteristics of youth, that are moving through space together with AB Dor. This diverse set of ∼50 m
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/87558
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Open clusters and associations: individual (AB Doradus moving group); Stars: kinematics; Stars: pre-main-sequence
dc.titleThe AB Doradus Moving Group
dc.typeJournal article
local.bibliographicCitation.lastpageL68
local.bibliographicCitation.startpageL65
local.contributor.affiliationZuckerman, B, University of California
local.contributor.affiliationSong, Inseok, Gemini Observatory
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidBessell, Michael, u6900904
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16902
local.identifier.citationvolume613
local.identifier.doi10.1086/425036
local.identifier.scopusID2-s2.0-7544228236
local.type.statusPublished Version

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