Type II supernovae - Analysis of the observed spectra from 8 to 15 months following the explosion

Details Type II supernovae - Analysis of the observed spectra from 8 to 15 months following the explosion Type II supernovae - Analysis of the observed spectra from 8 to 15 months following the explosion

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...220..484g&link_type=abstract

Astrophysical Journal, Part 1, vol. 220, Mar. 1, 1978, p. 484-489.

Astronomy and Astrophysics

Astrophysics

5

Astronomical Models, Astronomical Spectroscopy, Light Curve, Pulsars, Stellar Spectra, Supernovae, Envelopes, Explosions, Spectrum Analysis, Stellar Models

Scientific paper

A study of the spectra of two Type II supernovae, showing a slow
decrease in their light curve after approximately 100 days, has been
made. For these supernovae, at times greater than 100 days, the envelope
is shown to be ionized by radiation from a central source, probably a
pulsar. A tentative model of such an envelope is derived.

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