Non-LTE line formation in early B and late O stars. II - Equivalent widths for O II

Details Non-LTE line formation in early B and late O stars. II - Equivalent widths for O II Non-LTE line formation in early B and late O stars. II - Equivalent widths for O II

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74..211b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 2, Aug. 1988, p. 211-225.

Astronomy and Astrophysics

Astrophysics

23

B Stars, Nonequilibrium Thermodynamics, O Stars, Oxygen Spectra, Spectral Line Width, Stellar Spectra, Abundance, Atmospheric Models, Early Stars, Late Stars

Scientific paper

Equivalent widths for over 100 lines of O II in the 4000-5000 A
wavelength region have been calculated on a grid of B star model
atmospheres. The equivalent widths most important for abundance analyses
are presented. The calculative method utilized is briefly described.

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