On the helium abundance of Nova Cephei 1971 ejecta

Details On the helium abundance of Nova Cephei 1971 ejecta On the helium abundance of Nova Cephei 1971 ejecta

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186..617d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 186, Mar. 1979, p. 617-619.

Astronomy and Astrophysics

Astronomy

Abundance, Helium, Novae, Stellar Envelopes, Stellar Mass Ejection, Hydrogen, Line Spectra, Optical Thickness, Stellar Spectra

Scientific paper

A new analysis of the physical conditions of the shell ejected by Nova
Cephei 1971 has shown that optical depth effects are unimportant during
the evolutionary phases we have previously considered. The conclusion of
the present study is that He is overabundant in the nova ejecta.

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