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AbstractAbstract
[en] A numerical model has been created that produces self-consistent optical spectra, temperatures, and ionization states for a homologously expanding spherical shell which at t = 0 is assumed to consist of pure Nickel 56, and is further assumed to have density independent of radius within the shell. A brief summary is given of the model, followed by some results from the calculations
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Source
Apr 1980; 17 p; Supernova type I workshop; Austin, TX, USA; 17 - 19 Mar 1980; CONF-800370--1; Available from NTIS., PC A02/MF A01
Record Type
Report
Literature Type
Conference; Numerical Data
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