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A new density Variance-Mach number relation for subsonic and supersonic isothermal turbulence

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dc.contributor.authorKonstandin, Lukas
dc.contributor.authorGirichidis, Philipp
dc.contributor.authorFederrath, Christoph
dc.contributor.authorKlessen, Ralf Stephan
dc.date.accessioned2018-11-29T22:52:32Z
dc.date.available2018-11-29T22:52:32Z
dc.date.issued2012
dc.date.updated2018-11-29T07:46:55Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/152209
dc.publisherIOP Publishing
dc.sourceThe Astrophysical Journal
dc.subjectKeywords: hydrodynamics; ISM: kinematics and dynamics; ISM: structure; methods: numerical; shock waves; turbulence
dc.titleA new density Variance-Mach number relation for subsonic and supersonic isothermal turbulence
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage7
local.bibliographicCitation.startpage1
local.contributor.affiliationKonstandin, Lukas, University of Heidelberg
local.contributor.affiliationGirichidis, Philipp, University of Heidelberg
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationKlessen, Ralf Stephan, Ruprecht Karls University of Heidelberg
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.ariespublicationU3488905xPUB15091
local.identifier.citationvolume761
local.identifier.doi10.1088/0004-637X/761/2/149
local.identifier.scopusID2-s2.0-84870829994
local.identifier.thomsonID000312090300068
local.type.statusPublished Version

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