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Astrophysics and Space Science, 2003
In the coming years, a number of projects will start intensive supernov esearches resulting in an increase of the current statistics by a factor of 10. At low redshift, the Nearby Supernova Factory will detect and follow spectrophotometricly ~ 400 of SNe Ia with a redshift at z ~ 0.05, and improve our understanding of the intrinsic properties of SNe Ia.
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In the coming years, a number of projects will start intensive supernov esearches resulting in an increase of the current statistics by a factor of 10. At low redshift, the Nearby Supernova Factory will detect and follow spectrophotometricly ~ 400 of SNe Ia with a redshift at z ~ 0.05, and improve our understanding of the intrinsic properties of SNe Ia.
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SUPERNOVA EXPLOSIONS AND SUPERNOVA NEUTRINOS
Neutrinos in Physics and Astrophysics, 2000We summarize the current status of core-collapse supernova theory, in particular as it relates to multi-dimensional effects and neutrino transport . Highlighted are pulsar kicks , neutrino burst signatures, many-body effects, and observed asphericities that may have a bearing on the mechanism of supernova explosions .
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Supernovae and Supernova Remnants
1983Supernovae are the result of explosions which terminate the life of massive stars. The amount of energy released by the supernovae in our galaxy is so large that these explosions provide the dominant energy for the heating of the hot (T ≳ 106 K) IS component and for the kinetic energy of the large scale motions of the interstellar clouds.
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Supernovae and supernova remnants
2001A supernova explosion is among the most dramatic events that can be seen. The term ‘supernova’ is somewhat misleading, as such an event represents not a new star (that is, a ‘nova’), but instead the end of a star’s life. Nuclear fusion, the energy source of the stars, creates heavier elements from lighter elements.
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Supernovae And Supernova Remnants
Annual Review of Astronomy and Astrophysics, 1988Kurt W. Weiler, Richard A. Sramek
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