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dc.date.accessioned 2019-12-17T17:09:17Z
dc.date.available 2019-12-17T17:09:17Z
dc.date.issued 2017
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/87583
dc.description.abstract We present the first results of a detailed comparison between the pulsation properties of pulsating Extremely Low-Mass pre-white dwarf stars (the pre-ELMV variable stars) and δ Scuti stars. The instability domains of these very different kinds of stars nearly overlap in the log Teff vs. log g diagram, leading to a degeneracy in the classification of the stars. Our aim is to provide asteroseismic tools for their correct classification. en
dc.language en es
dc.subject Stars es
dc.subject pre-ELMV es
dc.title Comparing the asteroseismic properties of pulsating extremely low-mass pre-white dwarf stars and δ Scuti stars en
dc.type Articulo es
sedici.identifier.other doi:10.1051/epjconf/201715205008 es
sedici.identifier.other eid:2-s2.0-85029533861 es
sedici.identifier.issn 2101-6275 es
sedici.creator.person Sánchez Arias, Julieta Paz es
sedici.creator.person Córsico, Alejandro Hugo es
sedici.creator.person Romero, Alejandra Daniela es
sedici.creator.person Althaus, Leandro Gabriel es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.relation.event Wide-Field Variability Surveys: A 21st Century Perspective – 22nd Los Alamos Stellar Pulsation – Conference Series Meeting ( Chile, 28 de noviembre al 2 de diciembre de 2016) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle EPJ Web of Conferences es
sedici.relation.journalVolumeAndIssue vol. 152 es


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