The Evolution of Surface Parameters of Rotating Massive Stars
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We summarize the present status of the predictions of massive star models for the evolution of their surface properties. After discussing luminosity, temperature and chemical composition, we focus on the question whether massive stars may arrive at critical rotation during their evolution, either on the main sequence or in later stages. We find both cases to be possible and briefly discuss observable consequences.
8 pages, LaTeX, 3 PostScript figures (included), uses paspconf.sty (included), 1997, in: Proceeding of 2nd Boulder-Munich Workshop on Hot Stars, I. Howarth et al., eds, PASP Conf. Ser. Proc., 131, p. 76, also available at http://www.mpa-garching.mpg.de/Stars/Preprints/windsor.ps.gz
8 pages, LaTeX, 3 PostScript figures (included), uses paspconf.sty (included), 1997, in: Proceeding of 2nd Boulder-Munich Workshop on Hot Stars, I. Howarth et al., eds, PASP Conf. Ser. Proc., 131, p. 76, also available at http://www.mpa-garching.mpg.de/Stars/Preprints/windsor.ps.gz