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What probability distribution functions tell us about the processes of star formation

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dc.contributor.authorSchneider, N.
dc.contributor.authorOssenkopf, Volker
dc.contributor.authorKlessen, R.
dc.contributor.authorCsengeri, T.
dc.contributor.authorGirichidis, P.
dc.contributor.authorFederrath, Christoph
dc.contributor.authorTremblin, P
dc.contributor.authorBontemps, S.
dc.contributor.authorPeretto, N
dc.contributor.authorSimon, R
dc.contributor.editorSimon, R.
dc.contributor.editorSchaaf, R.
dc.contributor.editorStutzki, J.
dc.coverage.spatialTBC
dc.date.accessioned2024-07-26T01:03:39Z
dc.date.available2024-07-26T01:03:39Z
dc.date.created7 September 2015 through 11 September 2015
dc.date.issued2015
dc.date.updated2023-10-01T07:16:06Z
dc.description.abstractProbability distribution functions of column density (N-PDFs) are used to evaluate the relative importance of gravity, turbulence, magnetic fields, geometry, and radiative feedback governing the cloud's density structure and star-formation activity. These proce-sses influence the N-PDF and thus determine their shape, ranging from a purely lognormal distribution to one with power-law tail(s).
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.isbn9782759820221
dc.identifier.urihttps://hdl.handle.net/1885/733714205
dc.language.isoen_AUen_AU
dc.publisherConference Organising Committee
dc.relation.ispartofseries6th Zermatt Symposium on Conditions and Impact of Star Formation: From Lab to Space 2015
dc.rights© EAS, EDP Sciences, 2016
dc.sourceEAS Publications Series
dc.titleWhat probability distribution functions tell us about the processes of star formation
dc.typeConference paper
local.bibliographicCitation.lastpage176
local.bibliographicCitation.startpage175
local.contributor.affiliationSchneider, N., I. Physik. Institut
local.contributor.affiliationOssenkopf, Volker, Universität zu Köln (University of Cologne)
local.contributor.affiliationKlessen, R., Zentrum für Astronomie der Universität Heidelberg
local.contributor.affiliationCsengeri, T., Max-Planck Institut für Radioastronomie
local.contributor.affiliationGirichidis, P., MPA
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationTremblin, P, CEA Saclay
local.contributor.affiliationBontemps, S., Université Bordeaux
local.contributor.affiliationPeretto, N, Cardiff University
local.contributor.affiliationSimon, R, University of Cologne
local.contributor.authoruidFederrath, Christoph, u5575624
local.description.embargo2099-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor510100 - Astronomical sciences
local.identifier.absseo280120 - Expanding knowledge in the physical sciences
local.identifier.ariespublicationa383154xPUB3779
local.identifier.doi10.1051/eas/1575031
local.identifier.scopusID2-s2.0-84973896886
local.identifier.thomsonIDWOS:000377836300030
local.publisher.urlhttps://www.eas-journal.org/
local.type.statusPublished Version
publicationvolume.volumeNumber75-76

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