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dc.date.accessioned 2021-09-30T14:50:25Z
dc.date.available 2021-09-30T14:50:25Z
dc.date.issued 2010
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/125931
dc.description.abstract The line driven- and rotation modulated-wind theory predicts an alternative slow solution, besides from the standard m-CAK solution, when the rotational velocity is close to the critical velocity. We study the behaviour of the winds of A-type supergiants (Asg) and show that under particular conditions, e.g., when the δ line-force parameter is about 0.25, the slow solution could exist over the whole star, even for the cases when the rotational speed is slow or zero. We discuss density and velocity profiles as well as possible observational conterparts. en
dc.format.extent 184-185 es
dc.language en es
dc.subject Stars: supergiants es
dc.subject Stars: winds es
dc.subject Outflows es
dc.subject Stars: mass loss es
dc.title The Slow Winds of A-Type Supergiants en
dc.type Articulo es
sedici.identifier.other arXiv:1009.5350 es
sedici.identifier.other doi:10.1017/s1743921311010258 es
sedici.identifier.issn 1743-9213 es
sedici.identifier.issn 1743-9221 es
sedici.creator.person Granada, Anahí es
sedici.creator.person Curé, Michel es
sedici.creator.person Cidale, Lydia Sonia es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Astrofísica de La Plata 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


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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)