Off-Center Detonations in Evolved Stellar Cores

Details Off-Center Detonations in Evolved Stellar Cores Off-Center Detonations in Evolved Stellar Cores

Feb 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..26..391b&link_type=abstract

Astrophysics and Space Science, Volume 26, Issue 2, pp.391-401

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Recent work on late stages of evolution has raised the possibility that the stars in the mass range from 4 8M bd may ignite carbon violently off-center. Hydrodynamic evolution has been carried out for models with various central densities and for temperature profiles both with and without an inversion. It has been found that, provided ignition leads to a detonation, both types of presupernova models have essentially the same final post detonation behavior. In particular, an off-center detonation is unable to prevent a complete disruption of the star if ignition occurs at low density.

Affiliated with

Also associated with

No associations

Rating

Off-Center Detonations in Evolved Stellar Cores 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 Off-Center Detonations in Evolved Stellar Cores, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Off-Center Detonations in Evolved Stellar Cores will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1370778