On the star formation efficiency of turbulent magnetized clouds

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dc.contributor.authorFederrath, Christoph
dc.contributor.authorKlessen, Ralf S.
dc.date.accessioned2018-11-29T22:52:32Z
dc.date.available2018-11-29T22:52:32Z
dc.date.issued2013
dc.date.updated2018-11-29T07:46:51Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/152205
dc.publisherIOP Publishing
dc.sourceThe Astrophysical Journal
dc.subjectKeywords: ISM: clouds; ISM: kinematics and dynamics; ISM: structure; magnetohydrodynamics (MHD); stars: formation; turbulence
dc.titleOn the star formation efficiency of turbulent magnetized clouds
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage22
local.bibliographicCitation.startpage1
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationKlessen, Ralf S., Heidelberg University
local.contributor.authoremailu5575624@anu.edu.au
local.contributor.authoruidFederrath, Christoph, u5575624
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absfor020199 - Astronomical and Space Sciences not elsewhere classified
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB14475
local.identifier.citationvolume763
local.identifier.doi10.1088/0004-637X/763/1/51
local.identifier.scopusID2-s2.0-84872223766
local.identifier.thomsonID000313456700051
local.identifier.uidSubmittedByU3488905
local.type.statusPublished Version

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