Statistics – Computation
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..563t&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, June 1, 1990, p. 563-576. Research supported by th
Statistics
Computation
60
Computational Astrophysics, Stellar Evolution, Stellar Mass Ejection, Stellar Winds, Supernova Remnants, Bubbles, Explosions, H Alpha Line, Kinetic Energy, Wind Velocity, X Ray Astronomy
Scientific paper
Assuming spherical symmetry, numerical calculations are conducted for the evolution of supernova remnants resulting from explosions inside wind-driven bubbles excavated by the progenitor stars. The basic procedure and physical assumptions are outlined and a test calculation for a supernova explosion in a medium of constant density is presented. The calculations for the wind-driven bubbles show that the supernova ejecta generate a variety of reflected and transmitted shocks, a complex velocity field, and a variability in the time evolution of the X-ray and H-alpha emission. Also, it is found that the duration of the wind can affect the evolution of the supernova remnant.
Bodenheimer Peter
Franco Jose
Rozyczka Michal
Tenorio-Tagle Guillermo
No associations
LandOfFree
On the evolution of supernova remnants. I - Explosions inside pre-existing wind-driven bubbles does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the evolution of supernova remnants. I - Explosions inside pre-existing wind-driven bubbles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the evolution of supernova remnants. I - Explosions inside pre-existing wind-driven bubbles will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-988142