Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.301..405w&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 301, Issue 2, pp. 405-413.
Astronomy and Astrophysics
Astronomy
7
Nuclear Reactions, Nucleosynthesis, Abundances, Shock Waves, Supernovae: General
Scientific paper
An off-centre detonation propagating near the interface between a C-O core and a He envelope in a Type Ia supernova explosion is modelled as a steady two-dimensional similarity solution at a plane interface. We assume that in both regions the energy release occurs in an infinitely thin detonation, which produces material in nuclear statistical equilibrium (NSE) in He and in nuclear statistical quasi-equilibrium in C-O. An alpha-network is then used to determine the effect of the associated rarefaction wave in the C-O on the final abundance of intermediate elements. We find that, although there is a significant effect, the rarefaction is not strong enough to quench the reactions and prevent the C-O from burning to NSE.
Falle Sam A. E. G.
Sharpe Gary J.
Wiggins J. R. D.
No associations
LandOfFree
Double detonations at the core-envelope boundary in Type IA supernovae 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 Double detonations at the core-envelope boundary in Type IA supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Double detonations at the core-envelope boundary in Type IA supernovae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-762776