CNO abundances from pre-maximum spectra of Nova Cygni 1975

Details CNO abundances from pre-maximum spectra of Nova Cygni 1975 CNO abundances from pre-maximum spectra of Nova Cygni 1975

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..92..197s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 92, no. 1, May 1983, p. 197-202.

Astronomy and Astrophysics

Astrophysics

Abundance, Carbon, Nitrogen, Novae, Oxygen, Stellar Spectra, Absorption Spectra, Line Spectra, Spectrum Analysis, Stellar Atmospheres, Stellar Models

Scientific paper

Coudé spectra of Nova Cygni 1975 have been compared with LTE synthetic spectra and abundances derived for carbon, nitrogen, and oxygen. It was found that while carbon is not enhanced over the solar value, nitrogen and oxygen are substantially over-abundant by factors of at least 30 and 10, respectively. These results can be compared with analyses performed on the nebular spectrum.

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