Results 131 to 140 of about 6,394 (163)

The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant

open access: yes
Munoz-Sanchez G   +10 more
europepmc   +1 more source

Super Supernovae

Scientific American, 2012
The largest stars die in explosions more powerful than anyone thought possible—some triggered in part by the production of antimatter. ; © 2012 Scientific American, a division of Nature America, Inc. Published online: 15 May 2012.
openaire   +3 more sources

Intensive Supernovae Searches

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.
openaire   +1 more source

SUPERNOVA EXPLOSIONS AND SUPERNOVA NEUTRINOS

Neutrinos in Physics and Astrophysics, 2000
We 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

1983
Supernovae 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.
openaire   +1 more source

Supernovae and supernova remnants

2001
A 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.
openaire   +1 more source

Supernovae And Supernova Remnants

Annual Review of Astronomy and Astrophysics, 1988
Kurt W. Weiler, Richard A. Sramek
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SUPERNOVA THEORY

Nuclear Physics A, 1987
openaire   +1 more source

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