First detection of a low-mass stellar halo around the young open cluster η Chamaeleontis

dc.contributor.authorMurphy, Simon
dc.contributor.authorLawson, Warrick Andrew
dc.contributor.authorBessell, Michael
dc.date.accessioned2015-12-08T22:36:21Z
dc.date.issued2010
dc.date.updated2016-02-24T09:53:41Z
dc.description.abstractWe have identified several lithium-rich low-mass (0.08 < M < 0.3 M⊙) stars within 5°5 of the young open cluster η Chamaeleontis, nearly four times the radius of previous search efforts. Of these stars, we propose four new probable cluster members and
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/35214
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Open clusters and associations: individual: ? Chamaeleontis; Stars: kinematics and dynamics; Stars: pre-main sequence
dc.titleFirst detection of a low-mass stellar halo around the young open cluster η Chamaeleontis
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpageL54
local.bibliographicCitation.startpageL50
local.contributor.affiliationMurphy, Simon, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLawson, Warrick Andrew, University of New South Wales, ADFA
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu4203307@anu.edu.au
local.contributor.authoruidMurphy, Simon, u4203307
local.contributor.authoruidBessell, Michael, u6900904
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3356449xPUB122
local.identifier.citationvolume406
local.identifier.doi10.1111/j.1745-3933.2010.00879.x
local.identifier.scopusID2-s2.0-78649495122
local.identifier.thomsonID000279766800011
local.identifier.uidSubmittedByu3356449
local.type.statusPublished Version

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