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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.
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Abundances in supernova remnants

AIP Conference Proceedings, 1984
This paper outlines the abundances one may expect to observe as the result of an explosion of the evolved star that is the progenitor of a supernova. (AIP)
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Supernovae and Supernova Remnants

Annual Review of Astronomy and Astrophysics, 1988
Kurt W. Weiler, Richard A. Sramek
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Evolution of Supernova Remnants. I. Interacting Supernova Remnants

Publications of the Astronomical Society of Japan, 1978
Abstract The evolution and structure of two interacting supernova remnants (SNRs) are calculated by use of a time-dependent two-dimensional hydrodynamic code. The interactions of two SNRs are simulated in such a way that at a time t0 after the first supernova explosion, the second supernova explosion occurs at the distance D and two SNRs
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Supernovae and supernova remnants

1974
C. B. Cosmovici   +2 more
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Supernovae and Supernova Remnants

Annual Review of Astronomy and Astrophysics, 1964
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