Electron scattering and absorption-line formation in type II supernova atmospheres

Details Electron scattering and absorption-line formation in type II supernova atmospheres Electron scattering and absorption-line formation in type II supernova atmospheres

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..607s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Oct. 1982, p. 607-611) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Sept.-Oct.

Astronomy and Astrophysics

Astronomy

1

Absorption Spectra, Electron Scattering, Resonance Lines, Stellar Envelopes, Stellar Spectra, Supernovae, Monte Carlo Method, Opacity, Optical Thickness, Radiative Transfer, Scattering Functions, Stellar Atmospheres, Thomson Scattering

Scientific paper

Monte Carlo calculations have been performed for pure scattering line profiles originating in a supernova envelope that expands as v proportional to r. Electron scattering is taken into account. The anomalous 5892-A Na I profile in the spectrum of supernova 1970g is synthesized. The fact that its emission component is missing may be interpretable by a model which provides for electron scattering in the supernova atmosphere.

Affiliated with

Also associated with

No associations

Rating

Electron scattering and absorption-line formation in type II supernova atmospheres 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 Electron scattering and absorption-line formation in type II supernova atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Electron scattering and absorption-line formation in type II supernova atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1032077