Core-collapse Supernova Remnants
Core-Collapse Supernova Remnants is a subclass of supernova remnants originating specifically from the gravitational collapse of massive stars (>8 M☉) that undergo core-collapse supernovae, distinguished by their association with neutron stars or black holes, enrichment of heavy elements synthesized during the explosion, and characteristic expansion dynamics driven by the ejected stellar envelope interacting with the surrounding interstellar medium.
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A. V. Filippenko · Annual Review of Astronomy and Astrophysics · 1997 · 1.8K citations
Natural Sciences, Astronomy, Physics +13
H. A. Bethe · Reviews of Modern Physics · 1990 · 1.1K citations
Natural Sciences, Astronomy, Physics +17
Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows
Fabio Governato, Chris B. Brook, Lucio Mayer et al. · Nature · 2010 · 1K citations · Full text
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California Institute of Technology
Pasadena, United States
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206 publications
23.5K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
40 h-index
107 publications
6.8K citations
Max Planck Institute for Astrophysics
Garching, Germany
38 h-index
97 publications
12.7K citations
University of California, Berkeley
Berkeley, United States
38 h-index
128 publications
16.8K citations
The University of Tokyo
Tokyo, Japan
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246 publications
14.1K citations
Goddard Space Flight Center
Greenbelt, United States
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114 publications
7.2K citations

Centre National de la Recherche Scientifique
Paris, France
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281 publications
30.1K citations
Los Alamos National Laboratory
Los Alamos, United States
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ApJ · 358 publications · 28.2K citations
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PRD · 31 publications · 1.7K citations
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