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The impact of thermodynamics on gravitational collapse: Filament formation and magnetic field amplification

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dc.contributor.authorPeters, Thomas
dc.contributor.authorSchleicher, Dominik R. G.
dc.contributor.authorKlessen, R.
dc.contributor.authorBanerjee, Robi
dc.contributor.authorFederrath, Christoph
dc.contributor.authorSmith, Rowan J.
dc.contributor.authorSur, Sharanya
dc.date.accessioned2018-11-29T22:56:39Z
dc.date.available2018-11-29T22:56:39Z
dc.date.issued2012
dc.date.updated2018-11-29T08:13:31Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2041-8205
dc.identifier.urihttp://hdl.handle.net/1885/153588
dc.publisherInstitute of Physics Publishing Ltd.
dc.sourceAstrophysical Journal Letters
dc.subjectKeywords: ISM: general; ISM: kinematics and dynamics; ISM: magnetic fields; stars: formation
dc.titleThe impact of thermodynamics on gravitational collapse: Filament formation and magnetic field amplification
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage7
local.bibliographicCitation.startpage1
local.contributor.affiliationPeters, Thomas, Universitat Zurich
local.contributor.affiliationSchleicher, Dominik R. G., Institut fur Astrophysik Georg-August-Universitat
local.contributor.affiliationKlessen, R., Zentrum für Astronomie der Universität Heidelberg
local.contributor.affiliationBanerjee, Robi, Hamburger Sternwarte
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationSmith, Rowan J., University of Heidelberg
local.contributor.affiliationSur, Sharanya, Arizona State University
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.ariespublicationU3488905xPUB15071
local.identifier.citationvolume760
local.identifier.doi10.1088/2041-8205/760/2/L28
local.identifier.scopusID2-s2.0-84869181287
local.identifier.thomsonID000311103000009
local.type.statusPublished Version

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