NASA NTRS · 19870066753
Nonspherical supernova remnants. IV - Sequential explosions in OB associations
Abstract
Multisupernova remnants, driven by sequential supernova explosions in OB associations, are modelled by means of two-dimensional hydrodynamical calculations. It is shown that due to the Rayleigh-Taylor instability the remnants quickly evolve into highly irregular structures. A critical evaluation of the multisupernova model as an explanation for supershells is given.
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Tenorio-Tagle, G., Bodenheimer, P., Rozyczka, M.. 1987-08-01. Nonspherical supernova remnants. IV - Sequential explosions in OB associations. https://ntrs.nasa.gov/citations/19870066753
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