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Large Eddy Simulationen von isolierten Scheibengalaxien

dc.contributor.advisorNiemeyer, Jens Prof. Dr.
dc.contributor.authorBraun, Harald Udo
dc.date.accessioned2014-12-18T10:37:22Z
dc.date.available2014-12-18T10:37:22Z
dc.date.issued2014-12-18
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0023-996D-A
dc.identifier.urihttp://dx.doi.org/10.53846/goediss-4837
dc.description.abstractIn dieser Arbeit stelle ich ein neu entwickeltes, dynamisches Modell für das turbulente sternbildende interstellare Medium auf Skalen von einigen zehn Parsecs vor, welches den Namen MIST (Multi-phase Interstellar medium model with Star formation and Turbulence) trägt. Das Verhalten von MIST wurde mittels seiner Ein-Zonen-Gleichgewichtslösungen aber auch im Rahmen von Large Eddy Simulationen untersucht, wobei verschiedenste Beobachtungsresultate gleichzeitig reproduziert werden konnten.de
dc.language.isodeude
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/
dc.subject.ddc530de
dc.titleLarge Eddy Simulationen von isolierten Scheibengalaxiende
dc.typedoctoralThesisde
dc.title.translatedLarge Eddy Simulations of Isolated Disk Galaxiesde
dc.contributor.refereeSchmidt, Wolfram PD Dr.
dc.date.examination2014-12-05
dc.subject.gokPhysik (PPN621336750)de
dc.description.abstractengIn this thesis I present a newly developed, dynamical model for the turbulent, star-forming interstellar medium on scales of some ten parsecs, which is named MIST (Multi-phase Interstellar medium model with Star formation and Turbulence). The behavior of MIST was explored not only by means of its one-zone (quasi-) eqilibrium solutions but also in the framework of large eddy simulations of idealized isolated disk galaxies, where various observational findings could be reproduced simultaneously.de
dc.contributor.coRefereeSchleicher, Dominik Prof. Dr.
dc.subject.gerAstrophysikde
dc.subject.gerISMde
dc.subject.gerTurbulenzde
dc.subject.gerSternentstehungde
dc.subject.gernumerische Simulationde
dc.subject.gerGalaxiende
dc.subject.gerLESde
dc.subject.engastrophysicsde
dc.subject.engISMde
dc.subject.engturbulencede
dc.subject.engstar formationde
dc.subject.enggalaxiesde
dc.subject.engLESde
dc.subject.engsub-grid scale modelde
dc.subject.engnumerical simulationde
dc.identifier.urnurn:nbn:de:gbv:7-11858/00-1735-0000-0023-996D-A-9
dc.affiliation.instituteFakultät für Physikde
dc.identifier.ppn813035732


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