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The Energetics of Type II Supernovae
1984The energetics of type II supernovae is considered within the gravitational implosion-explosion picture. The total (internal plus gravitational) energies of different parts of the star are calculated, when they are in, or close to, hydrostatic equilibrium.
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Type II Supernovae Photospheres and Distances
1982The kinematical method of determining distances to supernovae is briefly reviewed. A program to compute the required continuum flux from model atmospheres of Type II supernovae is outlined. The results of a perturbed gray-body calculation are presented to indicate qualitatively some of the important features to be expected.
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Spectral Diagnostics og Type II Supernova
1991The investigation of the spectra of Type II supernovae (SN II) is important for different fields in astronomy and astrophysics. Firstly, SN II are one of the most luminous single objects and may reach the same brightness at maximum as a whole galaxy. Therefore, they can be used as candles (KIRSHNER and KWAN, [1]) to determine the distances of galaxies,
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Gamma-ray burst jets in supernovae
New Astronomy Reviews, 2021Alessandra Corsi, Davide Lazzati
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Surviving companions of Type Ia supernovae: theory and observations
New Astronomy Reviews, 2019Pilar Ruiz-Lapuente
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An asymmetric explosion as the origin of spectral evolution diversity in type Ia supernovae
Nature, 2010Maximilian Stritzinger +2 more
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Sub-luminous type Ia supernovae from the mergers of equal-mass white dwarfs with mass ∼0.9M⊙
Nature, 2010Rüdiger Pakmor +2 more
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