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dc.date.accessioned 2019-10-25T13:40:56Z
dc.date.available 2019-10-25T13:40:56Z
dc.date.issued 2011-07-12
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/84049
dc.description.abstract The Be star phenomenon is related to fast rotation, although the cause of this fast rotation is not yet clearly established. The basic effects of fast rotation on the stellar structure are reviewed: oblateness, mixing, anisotropic winds. The processes governing the evolution of the equatorial velocity of a single star (transport mechanisms and mass loss) are presented, as well as their metallicity dependence. The theoretical results are compared to observations of B and Be stars in the Galaxy and the Magellanic Clouds. en
dc.format.extent 62-72 es
dc.language en es
dc.subject Be es
dc.subject Outflows es
dc.subject Stars: emission-line es
dc.subject Stars: evolution es
dc.subject Stars: mass loss es
dc.subject Stars: rotation es
dc.subject Stars: winds es
dc.title Massive stellar models: rotational evolution, metallicity effects en
dc.type Articulo es
sedici.identifier.other http://dx.doi.org/10.1017/s1743921311009987 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Ekström, Sylvia es
sedici.creator.person Georgy, Cyril es
sedici.creator.person Meynet, Georges es
sedici.creator.person Maeder, André es
sedici.creator.person Granada, Anahí es
sedici.subject.materias Ciencias Astronómicas es
sedici.subject.materias Ciencias Exactas es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event IAU Symposium 272 (Paris, France, 19-23 July, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 6, no. S272 es
sedici.rights.sherpa * Color: verde* Pre-print del autor: si* Post-print del autor: si* Versión de editor/PDF:no* Condiciones:>>Author's Pre-print on author's personal website, departmental website, social media websites, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv>>Author's post-print on author's personal website on acceptance of publication>>Author's post-print on departmental website, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv, after a 6 months embargo>>La versión de editor/PDF no puede utilizarse>>Published abstract may be deposited>>El pre-print debe registrar la aceptación para su publicación>>Deben reconocerse el copyright y la fuente editorial>>Must link to publisher version or journal website>>Authors may choose to use a Creative Commons Attribution Non-Commercial No Derivatives License>>Publisher last reviewed on 09/10/2014* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1743-9213/es/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)