Rotation has a strong influence in the structure of stars. The centrifugal force caused by rotation produces a deformation of the star that also affects the profile of brightness at its surface, this is known as gravity darkening. In this chapter we will construct a simple model to predict the shape and surface brightness of a rotating star
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
Mechanisms influencing absorption line profiles of fast rotating stars can be sorted into two group...
Mechanisms influencing absorption line profiles of fast rotating stars can be sorted into two group...
International audienceIn this lecture I discuss the bulk surface heterogeneity of rotating stars, na...
International audienceIn this paper we develop a calculation code to account for the effects carried...
International audienceIn this paper we develop a calculation code to account for the effects carried...
International audienceIn this paper we develop a calculation code to account for the effects carried...
Context. Interpretation of interferometric observations of rapidly rotating stars requires a good mo...
Context. Interpretation of interferometric observations of rapidly rotating stars requires a good mo...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
In this paper we develop a calculation code to account for the effects carried by fast rotation on t...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
Mechanisms influencing absorption line profiles of fast rotating stars can be sorted into two group...
Mechanisms influencing absorption line profiles of fast rotating stars can be sorted into two group...
International audienceIn this lecture I discuss the bulk surface heterogeneity of rotating stars, na...
International audienceIn this paper we develop a calculation code to account for the effects carried...
International audienceIn this paper we develop a calculation code to account for the effects carried...
International audienceIn this paper we develop a calculation code to account for the effects carried...
Context. Interpretation of interferometric observations of rapidly rotating stars requires a good mo...
Context. Interpretation of interferometric observations of rapidly rotating stars requires a good mo...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
In this paper we develop a calculation code to account for the effects carried by fast rotation on t...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
International audienceContext. The interpretation of stellar apparent fundamental parameters (viewin...
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