Nonspherical supernova remnants. IV - Sequential explosions in OB associations

Details Nonspherical supernova remnants. IV - Sequential explosions in OB associations Nonspherical supernova remnants. IV - Sequential explosions in OB associations

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...182..120t&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 182, no. 1, Aug. 1987, p. 120-126. NASA-sponsored research.

Astronomy and Astrophysics

Astrophysics

46

B Stars, O Stars, Stellar Models, Stellar Structure, Supernova Remnants, Boundary Value Problems, Hydrodynamic Equations, Stellar Envelopes, Stellar Evolution, Taylor Instability, Two Dimensional Flow

Scientific paper

Multi-supernova 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 multi-supernova model as an explanation for supershells is given.

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