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dc.contributor.advisorDas, Mousumi
dc.contributor.authorKataria, Sandeep Kumar
dc.date.accessioned2020-12-11T10:21:05Z
dc.date.available2020-12-11T10:21:05Z
dc.date.submitted2019
dc.identifier.urihttps://etd.iisc.ac.in/handle/2005/4747
dc.description.abstractIn this thesis we have studied bar formation and evolution using N-body simulations. We have focused on the effect of bulge mass and concentration on bar formation and evolution, and derived a new bar formation criterion. We also tested the criterion with observations collected from literature. We then investigated the effect of bulge mass on bar pattern speed since observations do not give a clear idea of the nature and origin of slow and fast of bars in galaxies. Bars also a potential candidate for changing the dark matter profile in the central regions of galaxies as they transports angular momentum from disk to the dark halo. We have also studied this effect using N-body simulationsen_US
dc.language.isoen_USen_US
dc.relation.ispartofseries;G29641
dc.rightsI grant Indian Institute of Science the right to archive and to make available my thesis or dissertation in whole or in part in all forms of media, now hereafter known. I retain all proprietary rights, such as patent rights. I also retain the right to use in future works (such as articles or books) all or part of this thesis or dissertationen_US
dc.subjectGalaxyen_US
dc.subjectBar formationen_US
dc.subjectN-body simulationsen_US
dc.subject.classificationResearch Subject Categories::NATURAL SCIENCES::Physics::Astronomy and astrophysics::Galactical astronomyen_US
dc.titleThe Formation and Evolution of Bars, and Its Impact on Galaxy Dynamicsen_US
dc.typeThesisen_US
dc.degree.namePhDen_US
dc.degree.levelDoctoralen_US
dc.degree.grantorIndian Institute of Scienceen_US
dc.degree.disciplineFaculty of Scienceen_US


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