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a study on rotational and thermal properties

dc.contributor.authorJappsen, Anne-Katharina
dc.date.accessioned2010-10-12T18:25:35Z
dc.date.available2010-10-12T18:25:35Z
dc.date.issued2006
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0001-3102-9
dc.description.abstractWe investigate the rotational and thermal properties of star-forming molecular clouds using hydrodynamic simulations. Stars form from molecular cloud cores by gravoturbulent fragmentation. Understanding the angular momentum and the thermal evolution of cloud cores thus plays a fundamental role in completing the theoretical picture of star formation. This is true not only for current star formation as observed in regions like the Orion nebula or the ?-Ophiuchi molecular cloud but also for the formation of stars of the first or second generation in the universe...
dc.format.extent149 S.
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherUniv. Potsdam
dc.rights.urihttp://e-docs.geo-leo.de/rights
dc.subject.ddc523
dc.subject.gokTEG 000
dc.titlePresent and early star formation
dc.title.alternativea study on rotational and thermal properties
dc.typemonograph
dc.subject.gokverbalKosmogonie {Astronomie}
dc.identifier.doi10.23689/fidgeo-122
dc.identifier.ppn514202343
dc.type.versionpublishedVersion
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


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