Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2019-10-25T14:43:03Z
dc.date.available 2019-10-25T14:43:03Z
dc.date.issued 2010-10-05
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/84063
dc.description.abstract Be stars are thought to be fast rotating stars surrounded by an equatorial disc. The formation, structure and evolution of the disc are still not well understood. In the frame of single star models, it is expected that the surface of an initially fast rotating star can reach its keplerian velocity (critical velocity). The Geneva stellar evolution code has been recently improved, in order to obtain some estimates of the total mass loss and of the mechanical mass loss rates in the equatorial disc during the whole critical rotation phase. We present here the first results of the computation of a grid of fast rotating B stars evolving towards the Be phase, and discuss the first estimates we obtained. en
dc.format.extent 640-641 es
dc.language en es
dc.subject Be es
dc.subject Stars: emission-line es
dc.subject Stars: evolution es
dc.subject Stars: mass loss es
dc.subject Stars: rotation es
dc.title Equatorial mass loss from Be stars en
dc.type Articulo es
sedici.identifier.other http://dx.doi.org/10.1017/s1743921311011756 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Georgy, Cyril es
sedici.creator.person Ekström, Sylvia es
sedici.creator.person Granada, Anahí es
sedici.creator.person Meynet, Georges es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Comunicacion 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/


Descargar archivos

Thumbnail
Documento completo
Descargar archivo (202.0Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

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)