The Initial Mass Function and Young Brown Dwarf Candidates in NGC 2264. III. Photometric Data

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dc.contributor.authorSung, Hwankyung
dc.contributor.authorBessell, Michael
dc.contributor.authorChun, Moo-Young
dc.contributor.authorKarimov, Rivkat
dc.contributor.authorIbrahimov, Mansur
dc.date.accessioned2015-12-08T22:38:33Z
dc.date.issued2008
dc.date.updated2015-12-08T10:08:54Z
dc.description.abstractWe have performed deep wide-field CCD photometry of the young open cluster NGC 2264 to study the extent of star-forming regions (SFRs) and the shape of the initial mass function. In this paper, we present VRI and Hα photometry for more than 67,000 stars.
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/35860
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Open clusters and associations: individual (NGC 2264); Stars: low-mass, brown dwarfs; Stars: luminosity function, mass function
dc.titleThe Initial Mass Function and Young Brown Dwarf Candidates in NGC 2264. III. Photometric Data
dc.typeJournal article
local.bibliographicCitation.issueFeb
local.bibliographicCitation.lastpage466
local.bibliographicCitation.startpage441
local.contributor.affiliationSung, Hwankyung, Sejong University
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationChun, Moo-Young, Korea Astronomy and Space Science Institute
local.contributor.affiliationKarimov, Rivkat, Ulugh Beg Astronomical Institute
local.contributor.affiliationIbrahimov, Mansur, Ulugh Beg Astronomical Institute
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.ariespublicationu4362859xPUB129
local.identifier.citationvolume135
local.identifier.doi10.1088/0004-6256/135/2/441
local.identifier.scopusID2-s2.0-47249147183
local.identifier.thomsonID000253039700001
local.type.statusPublished Version

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