Oscillator strengths and NE abundance in B stars

Details Oscillator strengths and NE abundance in B stars Oscillator strengths and NE abundance in B stars

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...120..139m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 120, no. 1, April 1983, p. 139, 140. Research supported by the Consiglio Nazio

Astronomy and Astrophysics

Astrophysics

1

Abundance, B Stars, Neon, Oscillator Strengths, Nuclear Fusion, Stellar Evolution

Scientific paper

Using the STF method and the j-K coupling scheme the authors calculate the oscillator strengths for some Ne I lines of primary astrophysical interest, comparing them with other values given in the literature. The values appear systematically a little greater (mean difference ≅ +0.12) than those of other sources. The Ne abundance in B stars is then discussed in the light of these results.

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