The effects of convection on the colours of A and F stars

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dc.creatorSmalley, B.
dc.creatorKupka, F.
dc.date1998-05-06
dc.date.accessioned2026-07-07T02:26:48Z
dc.date.available2026-07-07T02:26:48Z
dc.descriptionWe present a discussion on the effects of convection on the uvby colours of A and F stars. The mixing-length theory used in ATLAS9 is compared to the turbulent convection theory of Canuto & Mazzitelli (1991, 1992). Comparison with fundamental stars reveals that colours calculated using the Canuto & Mazzitelli convection theory are generally in better agreement than those obtained using mixing-length theory.
dc.description5 pages, 2 figures, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schnell and J. Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No 3
dc.identifierhttps://arxiv.org/abs/astro-ph/9805058
dc.identifierhttp://arxiv.org/abs/astro-ph/9805058
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12428
dc.subjectAstrophysics
dc.titleThe effects of convection on the colours of A and F stars
dc.typetext

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