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The fragmentation of magnetized, massive star-forming cores with radiative feedback

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dc.contributor.authorMyers, Andrew T.
dc.contributor.authorMcKee, Christopher F.
dc.contributor.authorCunningham, Andrew J.
dc.contributor.authorKlein, Richard I.
dc.contributor.authorKrumholz, Mark
dc.date.accessioned2018-11-29T22:52:11Z
dc.date.available2018-11-29T22:52:11Z
dc.date.issued2013
dc.date.updated2018-11-29T07:44:27Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/152108
dc.publisherIOP Publishing
dc.sourceThe Astrophysical Journal
dc.subjectKeywords: ISM: clouds; magnetohydrodynamics (MHD); radiative transfer; stars: formation; stars: luminosity function, mass function; turbulence
dc.titleThe fragmentation of magnetized, massive star-forming cores with radiative feedback
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.contributor.affiliationMyers, Andrew T., University of California
local.contributor.affiliationMcKee, Christopher F., University of California
local.contributor.affiliationCunningham, Andrew J., Lawrence Livermore National Laboratory
local.contributor.affiliationKlein, Richard I., Lawrence Livermore National Laboratory
local.contributor.affiliationKrumholz, Mark, College of Science, ANU
local.contributor.authoruidKrumholz, Mark, u1000557
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationa383154xPUB3404
local.identifier.citationvolume766
local.identifier.doi10.1088/0004-637X/766/2/97
local.identifier.scopusID2-s2.0-84875436458
local.identifier.thomsonID000316320900031
local.type.statusPublished Version

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