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dc.date.accessioned 2024-07-04T14:14:03Z
dc.date.available 2024-07-04T14:14:03Z
dc.date.issued 2021
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/167764
dc.description.abstract Hot subdwarf stars are core helium-burning objects, located at the hot end of the horizontal branch, and therefore, they are also known as Extreme Horizontal Branch stars. We can divide them into two large groups, of spectral types B and O, depending on their effective temperature. Each spectroscopic class has subgroups showing luminosity variations due to pulsations, opening the possibility to study these compact objects through Asteroseismology. In this notes I will briefly review the main characteristics of hot subdwarfs B and O stars and the different pulsating subgroups. en
dc.format.extent 182-195 es
dc.language en es
dc.subject asteroseismology es
dc.subject instabilities es
dc.subject stars: oscillations es
dc.subject stars: interiors es
dc.title Pulsating Hot Subdwarf Stars en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-7-2 es
sedici.creator.person Romero, Alejandra Daniela 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) 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)