Non-LTE equivalent widths for SI II, III and IV

Astronomy and Astrophysics – Astrophysics

Scientific paper

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B Stars, Silicon, Spectral Line Width, Stellar Spectra, Abundance, Stellar Atmospheres, Stellar Models, Stellar Temperature, Thermodynamic Equilibrium

Scientific paper

Equivalent widths for a set of Si II, III, and IV lines reliable for the
determination of temperatures in the B star parameter range are given.
They are calculated on a line grid of LTE line-blanketed model
atmospheres and lie in the wavelength region from 4070 to 5070 A.

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