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From: YKhan on 25 May 2010 01:27 Supernova uncertainty "But the star's chemical composition doesn't fit with the model of an exploding white dwarf star either the material expelled in SN 2005E contains a higher fraction of calcium and titanium than any supernova observed so far. Instead, this signature is more typical of nuclear reactions involving helium, rather than the carbon and oxygen found in the centre of typical white dwarf stars. " http://www.astronomynow.com/news/n1005/20sn/ |