Irrigate 发表于 2025-3-25 04:28:24
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978-3-319-24149-4Springer International Publishing Switzerland 2016继承人 发表于 2025-3-25 14:30:21
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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 reviSTALL 发表于 2025-3-26 02:25:31
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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 presenDEMN 发表于 2025-3-26 14:32:03
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下船 发表于 2025-3-26 20:14:30
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