Mathematics – Logic
Scientific paper
Nov 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sscr.conf..221a&link_type=abstract
In: Supernovae: A survey of current research; Proceedings of the Advanced Study Institute, Cambridge, England, June 29-July 10,
Mathematics
Logic
20
Light Curve, Stellar Evolution, Stellar Models, Supernovae, Abundance, Black Body Radiation, Gamma Rays, Hubble Diagram, Nickel Isotopes, Opacity, Radiant Flux Density, Stellar Luminosity, Stellar Mass Ejection, Stellar Spectra
Scientific paper
The probable nature of supernovae is systematically analyzed using analytical models which are sufficiently general to include both Type I and II. Many aspects of the models are quantitatively compared with observations. A hypothetical blackbody supernova is analyzed in an attempt to obtain more detailed understanding of Type I supernovae, and an improved version of the distance and mass independent relation between gamma ray flux and observed apparent magnitude is given. Preliminary results for cosmological distance determination using supernovae are presented and expressed as a Hubble ratio. Implications for the energy, mass, composition, and preexplosion structure are summarized, and questions regarding dim supernovae and the pulsar and supernova rate, as well as iron production in supernovae are discussed.
No associations
LandOfFree
The nature of supernovae as determined from their light curves 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 The nature of supernovae as determined from their light curves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The nature of supernovae as determined from their light curves will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1759139