High explosive simulations of supernovae and the supernova shell fragmentation model of solar system formation

Details High explosive simulations of supernovae and the supernova shell fragmentation model of solar system formation High explosive simulations of supernovae and the supernova shell fragmentation model of solar system formation

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987stin...8811584b&link_type=abstract

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Computer Science

Evolution (Development), Explosions, Explosives, Simulation, Solar System, Stellar Models, Supernovae, Fragmentation, Photographs

Scientific paper

Comparison of photographs of explosive experiments to the Casseopeia A supernova remnant reveals a striking similarity. The similarity could indicate the presence of a relatively cool, underlying shell in the Casseopeia A remnant. As this shell expands and fragments, the observable features are produced by hot gases squirting through the cracks - as in explosive experiments. The existence of such underlying shells in supernova remnants supports the author's model of solar system formation.

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