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Metallicity and v sin i of B Stars in Galactic Open Clusters: is there any Correlation?
Published online by Cambridge University Press: 26 May 2016
Abstract
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We discuss the v sin i distributions of main sequence B stars in galactic clusters in relation to stellar luminosity and to cluster metallicity. We show that evolutionary effects and/or dependence of initial v sin i distribution on stellar mass are important, so that a much larger sample and a wider metallicity range are required to detect any possible metallicity effect beyond doubt.
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- Session 1 Observations of Rotating Stars
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- Copyright © Astronomical Society of the Pacific 2004
References
North, P., Royer, F., Melo, C., de Medeiros, J. R., do Nascimento, J. D. Jr., Mermilliod, J.-C., Grebel, E. K., Maeder, A., Mathieu, R.
2004, in Maeder, A. & Eenens, P. (eds.), Stellar Rotation, Proc. IAU Symp. No. 215 (San Francisco: ASP)Google Scholar
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