Exploració per tema "G41.1–0.3)— ISM: supernova remnants — nuclear reactions"
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A Chandrasekhar mass progenitor for the type Ia supernova remnant 3C 397 from the enhanced abundances of nickel and manganese
(2015-03-12)
Article
Accés restringit per política de l'editorialDespite decades of intense efforts, many fundamental aspects of Type Ia supernovae (SNe Ia) remain elusive. One of the major open questions is whether the mass of an exploding white dwarf (WD) is close to the Chandrasekhar ...