Comparing the asteroseismic properties of pulsating extremely low-mass pre-white dwarf stars and δ Scuti stars

dc.contributor.author	Sánchez Arias, J. P.	pt_BR
dc.contributor.author	Córsico, Alejandro Hugo	pt_BR
dc.contributor.author	Romero, Alejandra Daniela	pt_BR
dc.contributor.author	Althaus, Leandro Gabriel	pt_BR
dc.date.accessioned	2018-09-19T02:32:51Z	pt_BR
dc.date.issued	2017	pt_BR
dc.identifier.issn	2100-014X	pt_BR
dc.identifier.uri	http://hdl.handle.net/10183/182170	pt_BR
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.format.mimetype	application/pdf	pt_BR
dc.language.iso	eng	pt_BR
dc.relation.ispartof	EPJ Web of conferences. Les Ulis. Vol. 152 (2017), 05008, 2 p.	pt_BR
dc.rights	Open Access	en
dc.subject	Pulsacoes estelares	pt_BR
dc.subject	Anãs brancas	pt_BR
dc.subject	Asterosismologia	pt_BR
dc.title	Comparing the asteroseismic properties of pulsating extremely low-mass pre-white dwarf stars and δ Scuti stars	pt_BR
dc.type	Artigo de periódico	pt_BR
dc.identifier.nrb	001072888	pt_BR
dc.type.origin	Estrangeiro	pt_BR

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