Pulsating white dwarfs

dc.contributor.author	Kepler, Souza Oliveira	pt_BR
dc.contributor.author	Romero, Alejandra Daniela	pt_BR
dc.date.accessioned	2018-09-19T02:32:40Z	pt_BR
dc.date.issued	2017	pt_BR
dc.identifier.issn	2100-014X	pt_BR
dc.identifier.uri	http://hdl.handle.net/10183/182154	pt_BR
dc.description.abstract	The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor of five and consequently the number of known pulsating white dwarfs also by a factor of five. It has also led to the discovery of new types of variable white dwarfs, as the variable hot DQs, and the pulsating Extremely Low Mass white dwarfs. With the Kepler Mission, it has been possible to discover new phenomena, the outbursts present in a few pulsating white dwarfs.	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), 01011, 9 p.	pt_BR
dc.rights	Open Access	en
dc.subject	Anãs brancas	pt_BR
dc.subject	Pulsacoes estelares	pt_BR
dc.subject	Evolucao estelar	pt_BR
dc.title	Pulsating white dwarfs	pt_BR
dc.type	Artigo de periódico	pt_BR
dc.identifier.nrb	001072890	pt_BR
dc.type.origin	Estrangeiro	pt_BR

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