Comments on the spectrum of Nova Scuti 1975

Details Comments on the spectrum of Nova Scuti 1975 Comments on the spectrum of Nova Scuti 1975

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...221..211g&link_type=abstract

Astrophysical Journal, Part 1, vol. 221, Apr. 1, 1978, p. 211-219.

Astronomy and Astrophysics

Astrophysics

11

Abundance, Atomic Spectra, Emission Spectra, Line Spectra, Novae, Stellar Spectra, Helium, Hydrogen, Nitrogen, Optical Thickness, Oxygen Spectra

Scientific paper

Element abundances of Nova Scuti 1975 are examined by emission line spectra. It is noted that the Balmer decrement does not agree with predictions of case B recombination, and that the amount of interstellar extinction is not especially large. Elements for which abundance is recorded include O I, II, III; N I, II, III; H, and He I, and II. Alpha and beta hydrogen as well as He I are optically thick.

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