Titlebook: Cartography of the Sun and the Stars; Jean-Pierre Rozelot,Coralie Neiner Book 2016 Springer International Publishing Switzerland 2016 CHAR

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978-3-319-24149-4Springer International Publishing Switzerland 2016

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https://doi.org/10.1007/978-1-349-01327-2e stars as can be derived from their wide-band optical light curves. Spot modelling is becoming more and more important thanks to the high-precision, high duty-cycle photometric time series made available by space-borne telescopes designed to search for planets through the method of transits. I revi

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Outdoor Recreation Activities and Needs,lication of long-baseline interferometry to the determination of the photospheric shape of fast rotating stars. I present the example of the VLT Interferometer observations of the nearby Be star Achernar (.?Eri), using the VINCI (two telescopes) and PIONIER (four telescopes) beam combiners. I presen

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https://doi.org/10.1007/978-1-349-02079-9k of Michelson at the end of the XIXth—beginning of the XXth when he first resolved the surface of a star, Betelgeuse, with his colleague Pease. Images were obtained for the first time 20 years ago with the COAST instrument and interferometers have made constant progress to reach the minimum level w

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The Concession Gained and Lost, 1914–15st rotation velocities and thus those for which the consequences of rotation are the strongest. On the stellar photosphere fast-rotation induces (1) a geometrical flattening and (2) a non-uniform distribution of flux/effective temperature (gravity darkening effect). A detailed mapping of these effec