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Supernovae and Their Remnants [PDF]
, 1988 Supernovas can be divided into two distinct classes on the basis of their spectra. Supernovae of type I (SNI) exhibit no hydrogen lines whereas those of type II (SNII) do show hydrogen lines in their spectra. Historically (Baade 1958) SNI have, with the usual perversity of astronomical nomenclature, been assigned to Population II and SNII to Population
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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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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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Space Science Reviews, 1985
A progress report is given on our current interpretation of the X-ray emission from supernova remnants. Previous results from earlier experiments, the Einstein Observatory in particular, are reviewed and supplemented by the most recent data from the Exosat mission for a selection of remnants (Puppis-A, Cas-A, SN 1006, RCW103, W49B).
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A progress report is given on our current interpretation of the X-ray emission from supernova remnants. Previous results from earlier experiments, the Einstein Observatory in particular, are reviewed and supplemented by the most recent data from the Exosat mission for a selection of remnants (Puppis-A, Cas-A, SN 1006, RCW103, W49B).
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Observations of Supernova Remnants
Annual Review of Astronomy and Astrophysics, 1984Les restes de supernovae jeune: RSN riches en metaux CasA, restes de type I Tycho, le Crabe. Les restes d'âge intermediaire: la Boucle du Cygne. Les vieux restes de supernovae; l'eperon polaire nord. Les restes de supernovae de transition.
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1974
Supernovae of type II must be related to rather massive stars. They appear to occur rather exclusively in the spiral arms of galaxies and this fact alone sets a lower limit of about 5 M⊙ to their main sequence mass. If we believe that all massive stars above some critical value become supernovae (and none below this value) the supernova rate would ...
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Supernovae of type II must be related to rather massive stars. They appear to occur rather exclusively in the spiral arms of galaxies and this fact alone sets a lower limit of about 5 M⊙ to their main sequence mass. If we believe that all massive stars above some critical value become supernovae (and none below this value) the supernova rate would ...
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Supernovae and Supernova Remnants
Annual Review of Astronomy and Astrophysics, 1964openaire +2 more sources
Supernova Remnants: Supernova Remnants and Their X-Ray Emission.
Science, 1984openaire +3 more sources
An absence of ex-companion stars in the type Ia supernova remnant SNR 0509−67.5
Nature, 2012B. Schaefer, A. Pagnotta
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