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Modelling H2 formation in the turbulent interstellar medium: solenoidal versus compressive turbulent forcing

dc.contributor.authorMicic, Milica
dc.contributor.authorGlover, Simon C. O.
dc.contributor.authorFederrath, Christoph
dc.contributor.authorKlessen, R.
dc.date.accessioned2018-11-29T22:53:37Z
dc.date.available2018-11-29T22:53:37Z
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/152529
dc.format.mimetypeapplication/pdf
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.titleModelling H2 formation in the turbulent interstellar medium: solenoidal versus compressive turbulent forcing
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume421
dc.date.issued2012
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.ariespublicationU3488905xPUB14794
local.type.statusPublished Version
local.contributor.affiliationMicic, Milica, Zentrum fur Astronomie der Universitat Heidelberg
local.contributor.affiliationGlover, Simon C. O., Zentrum für Astronomie der Universität Heidelberg
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationKlessen, R., Zentrum für Astronomie der Universität Heidelberg
local.bibliographicCitation.issue3
local.bibliographicCitation.startpage2531
local.bibliographicCitation.lastpage2542
local.identifier.doi10.1111/j.1365-2966.2012.20477.x
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
dc.date.updated2018-11-29T07:53:50Z
local.identifier.scopusID2-s2.0-84859425021
local.identifier.thomsonID000302620500052
dcterms.accessRightsOpen Access
CollectionsANU Research Publications

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