Estimate of the ionization and mass of the envelopes of type I supernovae on the basis of the radioactive-decay hypothesis

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Cobalt Isotopes, Gas Ionization, Radioactive Decay, Stellar Envelopes, Stellar Mass Ejection, Supernovae, Free Electrons, Helium, Hydrogen, Iron, Kinetic Energy, Light Curve, Neutron Stars, Positrons, Stellar Evolution, Stellar Mass, Stellar Spectra

Scientific paper

An analysis of spectra of supernovae obtained in 1972 confirms the hypothesis that the radioactive decay of Ni-56 is responsible for the exponential portion of the light curves of type I supernovae. The interaction of positrons formed in the beta decay of Co-56 with matter ejected during the explosion of the envelope is studied, which makes is possible to determine the ionization of the envelope. It appears that the main source of free electrons in the envelope is helium, the most abundant of the elements there; iron tends to dominate the second stage of ionization. In this case, the mass of the envelope of 0.6 solar mass, and its kinetic energy is about 5 x 10 to the 50th erg. It is concluded that neutron stars are formed in the explosions of type I supernovae as well as in explosions of type II supernovae.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Estimate of the ionization and mass of the envelopes of type I supernovae on the basis of the radioactive-decay hypothesis 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 Estimate of the ionization and mass of the envelopes of type I supernovae on the basis of the radioactive-decay hypothesis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Estimate of the ionization and mass of the envelopes of type I supernovae on the basis of the radioactive-decay hypothesis will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1468753

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.