Establishing Super- and Sub-Chandrasekar Limiting Mass White Dwarfs to Explain Peculiar Type La Supernovae
A white dwarf is most likely the end stage of a low mass star like our Sun, which results when the parent star consumes all the hydrogen in its core, thus bringing fusion to a halt. It is a dense and compact object, where the inward gravitational pull is balanced by the outward pressure arising due...
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| Language: | en_US |
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2018
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| Online Access: | http://etd.iisc.ernet.in/2005/3752 http://etd.iisc.ernet.in/abstracts/4623/G26952-Abs.pdf |