The cooling wave in supernova shells

Details The cooling wave in supernova shells The cooling wave in supernova shells

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..44..409g&link_type=abstract

Astrophysics and Space Science, vol. 44, Oct. 1976, p. 409-428. Translation.

Astronomy and Astrophysics

Astrophysics

8

Stellar Envelopes, Stellar Mass Ejection, Stellar Temperature, Supernovae, Astrophysics, Cooling, Stellar Spectrophotometry

Scientific paper

A cooling wave apparently arises at some phases of supernova expansion. A number of basic properties of the cooling wave are considered. The dependence of light curve and color temperature on chemical composition and density distribution law has been investigated in detail. An estimate of the total mass ejected by type II supernovae leads to a maximum value of approximately 20 solar masses. The necessity of further careful spectroscopic and photometric observations at prolonged postmaximum phases, especially for type II supernovae, is emphasized.

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