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1989•Astronomy & Astrophysics Supplement SeriesRequires access

Chemical abundances in early B-type stars. I. Sample and metal line equivalent widths.

J. Werner Kilian, P. E. Nissen

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Abstract

Les observations spectrographiques de 21 etoiles jeunes de type B sont presentees. Les abondances stellaires sont etudiees. Les largeurs equivalentes de C, N, O, Ne, Mg, Al, Si, S et Fe sont determinees

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Les observations spectrographiques de 21 etoiles jeunes de type B sont presentees. Les abondances stellaires sont etudiees. Les largeurs equivalentes de C, N, O, Ne, Mg, Al, Si, S et Fe sont determinees

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Available abstract

Les observations spectrographiques de 21 etoiles jeunes de type B sont presentees. Les abondances stellaires sont etudiees. Les largeurs equivalentes de C, N, O, Ne, Mg, Al, Si, S et Fe sont determinees

Key concepts: Physics, Astrophysics, Stars, Line (geometry), Microturbulence, Astronomy, Geometry, Mathematics

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