Gamma-ray light curves and spectra for Type IA supernovae

Details Gamma-ray light curves and spectra for Type IA supernovae Gamma-ray light curves and spectra for Type IA supernovae

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...259..549h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 259, no. 2, p. 549-566.

Astronomy and Astrophysics

Astrophysics

27

Energy Storage, Gamma Ray Spectra, Light Curve, Stellar Spectra, Supernovae, Cobalt Isotopes, Mass Distribution, Nickel Isotopes, Stellar Models

Scientific paper

The gamma-ray energy deposition functions, light curves, and spectra have been computed for a set of theoretical Type Ia supernova models including deflagration, detonation, delayed detonation, and tamped detonation models. The results have been obtained with a Monte Carlo gamma-ray deposition scheme that takes all relevant gamma transitions and interaction processes into account. The computations demonstrate that Type Ia supernova models can be discriminated and that the absolute amount of Ni-56 synthesized in the event can be determined from the gamma-ray light curves and spectra.

Affiliated with

Also associated with

No associations

Rating

Gamma-ray light curves and spectra for 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 Gamma-ray light curves and spectra for Type IA supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-ray light curves and spectra for Type IA supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1199145