Analysis of information sources in references of the Wikipedia article "Supernova" in English language version.
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{{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help)SN 1961V in NGC 1058 (Type V) had the most bizarre light curve ever recorded
Theoretical models of SNIa have remained limited because of uncertainties in the explosion mechanisms. [...] SNIa explosions are driven by fast thermonuclear burning in 12
C/15
O white dwarf (WD) stars with a mass close to, or below, the Chandrasekhar mass limit of ≈1.4 solar masses [...] Beyond this general statement, however, the exact mechanisms of SNIa remain unclear, with a number of possible scenarios.
{{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite book}}: Cite uses deprecated parameter |citeseerx= (help)Theoretical models of SNIa have remained limited because of uncertainties in the explosion mechanisms. [...] SNIa explosions are driven by fast thermonuclear burning in 12
C/15
O white dwarf (WD) stars with a mass close to, or below, the Chandrasekhar mass limit of ≈1.4 solar masses [...] Beyond this general statement, however, the exact mechanisms of SNIa remain unclear, with a number of possible scenarios.
{{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite book}}: Cite uses deprecated parameter |citeseerx= (help)SN 1961V in NGC 1058 (Type V) had the most bizarre light curve ever recorded
Theoretical models of SNIa have remained limited because of uncertainties in the explosion mechanisms. [...] SNIa explosions are driven by fast thermonuclear burning in 12
C/15
O white dwarf (WD) stars with a mass close to, or below, the Chandrasekhar mass limit of ≈1.4 solar masses [...] Beyond this general statement, however, the exact mechanisms of SNIa remain unclear, with a number of possible scenarios.
{{cite journal}}: Cite uses deprecated parameter |citeseerx= (help)Theoretical models of SNIa have remained limited because of uncertainties in the explosion mechanisms. [...] SNIa explosions are driven by fast thermonuclear burning in 12
C/15
O white dwarf (WD) stars with a mass close to, or below, the Chandrasekhar mass limit of ≈1.4 solar masses [...] Beyond this general statement, however, the exact mechanisms of SNIa remain unclear, with a number of possible scenarios.
{{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite book}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help)In 1980, Ken'ichi Nomoto of the University of Tokyo predicted a third type called an electron capture supernova. ... In an electron capture supernova, as the core runs out of fuel, gravity forces electrons in the core into their atomic nuclei, causing the star to collapse in on itself.
{{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite book}}: Cite uses deprecated parameter |citeseerx= (help)Theoretical models of SNIa have remained limited because of uncertainties in the explosion mechanisms. [...] SNIa explosions are driven by fast thermonuclear burning in 12
C/15
O white dwarf (WD) stars with a mass close to, or below, the Chandrasekhar mass limit of ≈1.4 solar masses [...] Beyond this general statement, however, the exact mechanisms of SNIa remain unclear, with a number of possible scenarios.
{{cite journal}}: Cite uses deprecated parameter |citeseerx= (help){{cite journal}}: Cite uses deprecated parameter |citeseerx= (help)In 1980, Ken'ichi Nomoto of the University of Tokyo predicted a third type called an electron capture supernova. ... In an electron capture supernova, as the core runs out of fuel, gravity forces electrons in the core into their atomic nuclei, causing the star to collapse in on itself.
SN 1961V in NGC 1058 (Type V) had the most bizarre light curve ever recorded
Theoretical models of SNIa have remained limited because of uncertainties in the explosion mechanisms. [...] SNIa explosions are driven by fast thermonuclear burning in 12
C/15
O white dwarf (WD) stars with a mass close to, or below, the Chandrasekhar mass limit of ≈1.4 solar masses [...] Beyond this general statement, however, the exact mechanisms of SNIa remain unclear, with a number of possible scenarios.