Spectrophotometric properties of pre-main-sequence stars:the ɛ Chamaeleontis cluster

dc.contributor.authorLyo, A.-Ran
dc.contributor.authorLawson, Warrick Andrew
dc.contributor.authorBessell, Michael
dc.date.accessioned2015-12-08T22:37:38Z
dc.date.issued2008
dc.date.updated2015-12-08T10:01:10Z
dc.description.abstractWe present a study of flux-calibrated low-resolution optical spectroscopy of 10 stars belonging to eight systems in the ∼5-Myr-old ε Chamaeleontis (ε Cha) pre-main-sequence (PMS) star cluster. Using synthetic broad-band colours, narrow-band continuum,
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/35607
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Open clusters and associations: individual: e Chamaeleontis; Stars: fundamental parameters; Stars: pre-main-sequence
dc.titleSpectrophotometric properties of pre-main-sequence stars:the ɛ Chamaeleontis cluster
dc.typeJournal article
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage1469
local.bibliographicCitation.startpage1461
local.contributor.affiliationLyo, A.-Ran, Korea Astronomy and Space Science Institute
local.contributor.affiliationLawson, Warrick Andrew, University of New South Wales, ADFA
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu6900904@anu.edu.au
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.ariespublicationu4362859xPUB126
local.identifier.citationvolume389
local.identifier.doi10.1111/j.1365-2966.2008.13688.x
local.identifier.scopusID2-s2.0-51349123996
local.identifier.thomsonID000259087500046
local.identifier.uidSubmittedByu4362859
local.type.statusPublished Version

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