Massive stars, successes and challenges

Article Article scientifique Article Massive stars, successes and challenges eng 2017-07-28 2016-11 author Meynet Georges 22422 Département d'astronomie (ASTRO) author Maeder André 25143 Administration de la faculté des sciences (SIAD) author Georgy Cyril 0000-0003-2362-4089 540258 Département d'astronomie (ASTRO) author Ekström Sylvia 0000-0002-2564-5660 514725 Département d'astronomie (ASTRO) author Eggenberger Patrick 0000-0001-6319-9297 504578 Département d'astronomie (ASTRO) author Barblan Fabio 26892 author Song Hanfeng 784889 Département d'astronomie (ASTRO) 3-14 10.1017/s1743921317003283 1743-9213 https://www.cambridge.org/core/product/identifier/S1743921317003283/type/journal_article We give a brief overview of where we stand with respect to some old and new questions bearing on how massive stars evolve and end their lifetime. We focus on the following key points that are further discussed by other contributions during this conference: convection, mass losses, rotation, magnetic field and multiplicity. For purpose of clarity, each of these processes are discussed on its own but we have to keep in mind that they are all interacting between them offering a large variety of outputs, some of them still to be discovered. Dewey 520 26 Département d'astronomie 12 false Proceedings of the International Astronomical Union 12 S329 17f6de52-6e01-4bda-9323-286c799c7563 Article (Published version) Restricted Article_scientifique_from_crossref(.pdf 332041 application/pdf 390954ec938eac567091f17add24b108db47f70001a32e69e478dcf082f03336 restrictedAccess Faculté des sciences / Département d'astronomie

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Massive stars, successes and challenges	Proceedings of the International Astronomical Union			2016	1	0

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Song, Hanfeng