Non-spherical collapse of a radiating star

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dc.contributor.authorGhosh, S. G.
dc.contributor.authorDeshkar, D. W.
dc.date.accessioned2012-03-13T09:09:28Z
dc.date.available2012-03-13T09:09:28Z
dc.date.issued2002-04-01
dc.description.abstractWe study the junction conditions for non-spherical (plane symmetric) collapsing ra- diating star consisting of a shearing fluid undergoing radial heat flow with outgoing radiation. Radiation of the system is described by plane symmetric Vaidya solution. Physical quantities relating to the local conservation of momentum and surface red-shift are also obtained.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1382
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprints;39/02
dc.subjectNon-spherical collapsingen_US
dc.subjectRa- diating staren_US
dc.titleNon-spherical collapse of a radiating staren_US
dc.typeArticleen_US

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