Zobrazeno 1 - 2
of 2
pro vyhledávání: '"F. C. De Gerónimo"'
Publikováno v:
Proceedings of the International Astronomical Union. 15:110-113
Ultra-massive (⩾M⊙) oxygen/neon (ONe) core white dwarfs (WDs) are the result of the evolution of isolated progenitor stars with masses above 6−M⊙. It is expected that hydrogen-rich (DA) ultra-massive WDs harbor crystallized cores at the typic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c816c6c0e7ed6053c046917584eb7822
https://doi.org/10.1017/s1743921320001362
https://doi.org/10.1017/s1743921320001362
Autor:
Alejandra D. Romero, Leandro Gabriel Althaus, Souza Oliveira Kepler, Barbara G. Castanheira, Alexandros Gianninas, D. Koester, Adela Kawka, Alejandro H. Córsico, C. Bonato, F. C. De Gerónimo, J. J. Hermes
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Universidad Nacional de La Plata
instacron:UNLP
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We present an asteroseismological analysis of four ZZ Ceti stars observed with the Kepler spacecraft: GD 1212, SDSS J113655.17+040952.6, KIC 11911480, and KIC 4552982, based on a grid of full evolutionary models of DA white dwarf (WD) stars. We emplo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9096078cb93dad771b2f9492a60eac5a
