The nitrogen abundance in Wolf-Rayet WC stars

Details The nitrogen abundance in Wolf-Rayet WC stars The nitrogen abundance in Wolf-Rayet WC stars

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...154..100n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 154, no. 1-2, Jan. 1986, p. 100-102.

Astronomy and Astrophysics

Astrophysics

2

Nitrogen, Stellar Composition, Stellar Evolution, Wolf-Rayet Stars, Absorption Spectra, Iue, Stellar Spectra

Scientific paper

In order to confirm the presence of nitrogen in WC stars, the IUE spectra of the WC 8 star HD 192103 have been studied in the region 1230-1250 A. The fluxes in the spectra of HD 192103 were extracted using two different procedures: the method described by Ramella et al. (1983); and the background correction method of Schmutz (1985). It is demonstrated that there is no convincing evidence of NV 2s 2S1/2-2p 2P(0)3/2 absorption at 1238.8 A in the spectrum of WC 192103.

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