Theoretical models for the continuum and colors of SN 1979 C and SN 1980 K

Details Theoretical models for the continuum and colors of SN 1979 C and SN 1980 K Theoretical models for the continuum and colors of SN 1979 C and SN 1980 K

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...210..262h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 210, no. 1-2, Feb. 1989, p. 262-272.

Astronomy and Astrophysics

Astrophysics

8

Astronomical Models, Spectral Energy Distribution, Stellar Color, Stellar Evolution, Supernovae, Abundance, Balmer Series, Color-Color Diagram, Continuous Radiation, Radiative Transfer, Stellar Envelopes

Scientific paper

Models for the continuum energy distribution from supernovae of type II are constructed and compared with the recently observed SN 1979 C and SN 1980 K for the coasting phase of their evolution. Fairly good agreement with the observed energy distributions from the UV range down to the IR as well as with colors is found. Using the colors, it is demonstrated how the distance to the SN can be found. The advantage of this method relative to the classical Baade-Wesselink method is that it needs data only for a single time.

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