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Radiatively efficient magnetized Bondi accretion

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dc.contributor.authorCunningham, Andrew J.
dc.contributor.authorMcKee, Christopher F.
dc.contributor.authorKlein, Richard I.
dc.contributor.authorKrumholz, Mark
dc.contributor.authorTeyssier, R
dc.date.accessioned2018-11-29T22:52:13Z
dc.date.available2018-11-29T22:52:13Z
dc.date.issued2012
dc.date.updated2018-11-29T07:44:43Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/152116
dc.publisherIOP Publishing
dc.sourceThe Astrophysical Journal
dc.subjectKeywords: ISM: magnetic fields; magnetohydrodynamics (MHD); stars: formation
dc.titleRadiatively efficient magnetized Bondi accretion
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.contributor.affiliationCunningham, Andrew J., Lawrence Livermore National Laboratory
local.contributor.affiliationMcKee, Christopher F., University of California
local.contributor.affiliationKlein, Richard I., Lawrence Livermore National Laboratory
local.contributor.affiliationKrumholz, Mark, College of Science, ANU
local.contributor.affiliationTeyssier, R, CEA, IRFU
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.ariespublicationa383154xPUB3416
local.identifier.citationvolume744
local.identifier.doi10.1088/0004-637X/744/2/185
local.identifier.scopusID2-s2.0-84555188088
local.identifier.thomsonID000298666400104
local.type.statusPublished Version

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