Gas Mass Loss of Dwarf Galaxies in Galaxy Clusters

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dc.contributor.authorSingh, Gagan Preet
dc.date.accessioned2013-06-15T14:58:51Z
dc.date.available2013-06-15T14:58:51Z
dc.date.issued2013-06-05
dc.description.abstractThis thesis looks at the interactions between galaxies within a galaxy cluster and discusses the mechanisms by which masses and sizes of these galaxies evolve. The processes discussed are Tidal Interactions, Dynamical Friction and Ram Pressure Stripping. The primary purpose of this thesis is to find out a relationship that tells us how small galaxies revolving around larger galaxies lose their gas content.en_US
dc.guideBagla, J.S.
dc.identifier.urihttp://hdl.handle.net/123456789/302
dc.language.isoenen_US
dc.publisherIISER Men_US
dc.subjectPhysicsen_US
dc.subjectGalaxyen_US
dc.titleGas Mass Loss of Dwarf Galaxies in Galaxy Clustersen_US
dc.typeThesisen_US

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