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dc.date.accessioned 2024-07-04T14:20:48Z
dc.date.available 2024-07-04T14:20:48Z
dc.date.issued 2021
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/167765
dc.description.abstract The post-main sequence evolution of massive stars still bears many unknowns. In particular, the physical processes involved in triggering enhanced mass-loss or eruptions are yet to be established. In this Chapter, the post-main sequence evolution of massive stars, and the various phases which are well-known for their mass ejections, are briefly touched upon. Amongst those transition phases, two classes of objects are discussed in more detail: the B-type supergiants and the Yellow Hypergiants. Their ability to perform pulsations is presented based on observational and theoretical evidences. Moreover, the possibility of a pulsation-mass-loss relation in these two classes of objects is delineated. en
dc.format.extent 234-254 es
dc.language en es
dc.subject asteroseismology es
dc.subject instabilities es
dc.subject stars: oscillations es
dc.subject stars: winds, outflows es
dc.title Pulsations in Evolved Massive Stars en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-7-2 es
sedici.creator.person Kraus, Michaela es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Objeto de conferencia 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.date.exposure 2019-11
sedici.relation.event VIII La Plata International School: Pulsations Along Stellar Evolution (La Plata, 11 al 22 de noviembre de 2019) es
sedici.description.peerReview peer-review es
sedici.relation.bookTitle Pulsations Along Stellar Evolution: Proceedings of the VIII La Plata International School es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)