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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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Abundances in supernova remnants
AIP Conference Proceedings, 1984This 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, 1988Kurt W. Weiler, Richard A. Sramek
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Evolution of Supernova Remnants. I. Interacting Supernova Remnants
Publications of the Astronomical Society of Japan, 1978Abstract 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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Supernova Remnants: Supernova Remnants and Their X-Ray Emission.
Science, 1984openaire +2 more sources
Supernovae and Supernova Remnants
Annual Review of Astronomy and Astrophysics, 1964openaire +1 more source
An absence of ex-companion stars in the type Ia supernova remnant SNR 0509−67.5
Nature, 2012Ashley Pagnotta
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