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Spectroscopic Analyses of Hot Main Sequence Stars

Published online by Cambridge University Press:  12 April 2016

Kozo Sadakane
Kozo Sadakane*
Affiliation:
Astronomical Institute, Osaka kyoiku UniversityTennoji-ku, Osaka, Japan543

Abstract

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Spectroscopic studies of normal O and early B type stars in the visual region are discussed. Present status of UV spectroscopic analyses of hot normal stars is reviewed. Discussions on a few practical problems in analyses of UV spectra are presented.

Type
Section IV - Non-Magnetic CP and Related Stars
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 369 - 380
Copyright
Copyright © Reidel 1986

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