Temperature Variations in Star Forming Interstellar Cloud Cores

A tétel rövid nézete
dc.contributor.advisorNándori, István
dc.contributor.authorKushwahaa, Tanya
dc.contributor.departmentDE--Természettudományi és Technológiai Kar--Fizikai Intézethu_HU
dc.date.accessioned2020-05-14T08:51:39Z
dc.date.available2020-05-14T08:51:39Z
dc.date.created2020-05-12
dc.description.abstractIn my dissertation, I have analysed the ammonia observations and the derived physical parameters of 36 Planck Galactic Cold Clumps, to search for systematic correlations between the calculated densities (NH3 column density, H2 volume density) and temperatures (excitation, rotation and kinetic temperatures) in the gas. The comparison of these parameters may imply the evolutionary state of these objects and reveal the differences and common signatures in the star formation process in different environments.hu_HU
dc.description.correctorSz.G.
dc.description.coursePhysicshu_HU
dc.description.degreeBSc/BAhu_HU
dc.format.extent61hu_HU
dc.identifier.urihttp://hdl.handle.net/2437/287183
dc.language.isoenhu_HU
dc.subjectStar Formationhu_HU
dc.subjectPlanck Galactic Cold Clumps
dc.subjectAstronomy
dc.subject.dspaceDEENK Témalista::Fizikahu_HU
dc.titleTemperature Variations in Star Forming Interstellar Cloud Coreshu_HU
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Theses (Faculty of Science and Technology)