... This achromaticity and the simultaneity at both sides of # c rules out other explanations such as a density fluctuation, a dust echo or a supernova bump (which could also be ruled out by amplitude and onset time). ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2007/A&A_462_L57.ps -- 942.0 Кб -- 24.02.2010 Похожие документы
... Nor has it been determined whether the carbonoxygen white dwarf in the system is able to accumulate mass due to accretion from its cool companion until it approaches the Chandrasekhar limit and becomes a supernova SN Ia progenitor. ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2007/AstBu_62_339.pdf -- 549.1 Кб -- 24.02.2010 Похожие документы
... optical afterglow of GRB970508 revisited: another case for GRB-Supernova connection", Abstracts of JENAM-2000, 2000, p. 190 [31 ... 49, 5-13 [33] Sokolov V.V. "Evidence for a Supernova in the I c Band Light Curve of the Optical Transient of GRB 970508 ...