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Long Baseline Interferometry of Rotating Stars Across the HR Diagram: Flattening, Gravity Darkening, Differential Rotation

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The Rotation of Sun and Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 765))

Abstract

Stellar rotation has been for a long time considered as a second-order effect on theories of stellar structure and evolution. Modern observations proved that stellar rotation is a key parameter to explain many physical mechanisms on stars. In particular optical/IR long baseline interferometry (OLBI) became a key technique to study stellar rotation across the HR diagram. In this contribution we describe the most important OLBI results obtained in the field of stellar rotation since the beginning of the twenty-first century.

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Author information

Authors and Affiliations

  1. Lab. H. Fizeau CNRS UMR 6525, Univ. de Nice-Sophia Antipolis Observatoire de la Côte d’Azur, 06108 Nice Cedex 2, France

    A. Domiciano de Souza

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  1. A. Domiciano de Souza
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Editors and Affiliations

  1. Dept. Fizeau, Université de Nice Sophia-Antipolis CNRS-OCA, av. Copernic, 06130, Grasse, France

    Jean-Pierre Rozelot

  2. Observatoire de Paris Section de Meudon GEPI, 5 place Jules Janssen, 92195, Meudon CX, France

    Coralie Neiner

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Souza, A.D.d. (2009). Long Baseline Interferometry of Rotating Stars Across the HR Diagram: Flattening, Gravity Darkening, Differential Rotation. In: Rozelot, JP., Neiner, C. (eds) The Rotation of Sun and Stars. Lecture Notes in Physics, vol 765. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-87831-5_7

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