An atlas of calculated continuum energy distributions for supernovae of type II

Details An atlas of calculated continuum energy distributions for supernovae of type II An atlas of calculated continuum energy distributions for supernovae of type II

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...77..115h&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 77, no. 1, Jan. 1989, p. 115-123. Research supported by the

Astronomy and Astrophysics

Astrophysics

2

Spectral Energy Distribution, Stellar Envelopes, Supernovae, Astronomical Spectroscopy, Boltzmann Distribution, Gas Pressure, Photosphere, Stellar Atmospheres

Scientific paper

An atlas of continuum energy distributions in the UV, visible, and near-IR regions has been compiled for type II supernovae. It is assumed that the cooling envelope can be approximated with a sequence of stationary atmospheres, that the level populations follow a Boltzmann distribution for the local temperature throughout the photosphere, and that the strongest source of continuum opacity is electron scattering. Results are presented for models with effective temperatures of between 7000 and 15,000 K.

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