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

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

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...76..331b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 76, no. 3, Dec. 1988, p. 331-338.

Astronomy and Astrophysics

Astrophysics

21

B Stars, Nitrogen Ions, Nonequilibrium Thermodynamics, O Stars, Spectral Line Width, Stellar Spectra, Energy Levels, Stellar Atmospheres, Tables (Data)

Scientific paper

A grid of non-LTE equivalent widths for 33 lines of N II in the
wavelegnth region from 4000 A to 5000 A is presented. These equivalent
widths are calculated in B-star line-blanketed model atmospheres. The
transitions and wavelength and integration ranges used in the
determination of the equivalent widths are listed.

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