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Physical Processes Leading to Surface Inhomogeneities: The Case of Rotation

Abstract : In this lecture I discuss the bulk surface heterogeneity of rotating stars, namely gravity darkening. I especially detail the derivation of the ω-model of Espinosa Lara and Rieutord (Astron Astrophys 533:A43, 2011), which gives the gravity darkening in early-type stars. I also discuss the problem of deriving gravity darkening darkening in stars owning a convective envelope and in those that are members of a binary system.
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https://hal-insu.archives-ouvertes.fr/insu-03675417
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Submitted on : Monday, May 23, 2022 - 10:28:25 AM
Last modification on : Monday, July 4, 2022 - 8:53:54 AM

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Michel Rieutord. Physical Processes Leading to Surface Inhomogeneities: The Case of Rotation. 2016, pp.101. ⟨10.1007/978-3-319-24151-7_5⟩. ⟨insu-03675417⟩

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