The chemical composition of the Nova Cephei 1971 ejecta

Details The chemical composition of the Nova Cephei 1971 ejecta The chemical composition of the Nova Cephei 1971 ejecta

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.181..421d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 181, Nov. 1977, p. 421-426.

Astronomy and Astrophysics

Astronomy

7

Chemical Composition, Novae, Stellar Mass Ejection, Thermonuclear Reactions, Abundance, Carbon, Helium, Nitrogen, Oxygen Spectra

Scientific paper

The chemical composition of the Nova Cephei 1971 ejecta was obtained
from analysis of the emission lines. He, O and N are overabundant with
respect to the cosmic values, consistent with the CNO thermonuclear
runaway. The ejected shell has a mass of about 0.0001 solar mass.

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