Asteroseismology of the ZZ Ceti and DAZ GD 133

Authors :: Fu, J.-N.
Vauclair, Gérard
Su, J.
Cang, T.
Li, C.
Xue, H.
Jiang, X.-J.
Li, Y.
Niu, H.
Zhang, X.
Colas, François
Dolez, N.
Fox Machado, L.
Michel, R.
Alvarez, M.
Kim, S.-L.
Department of Astronomy and Space Science, Chungnam National University
Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)
Astéroïdes, comètes, météores et éphémérides (ACME)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Tremblay
P.-E.
Gaensicke
B.
Marsh
T.
Source :: ASP Conference series, 20th European White Dwarf Workshop, 20th European White Dwarf Workshop, Jul 2016, University of Warwick, Coventry, West Midlands, United Kingdom, United Kingdom. pp.355
Publication Year :: 2016
Publisher :: HAL CCSD, 2016.
Abstract: International audience; GD 133 is a DAZ white dwarf with an atmosphere polluted by heavy elements accreted from a debris disk, which is formed by the disruption of rocky planetesimals

Language :: English
Database :: OpenAIRE
Journal :: ASP Conference series, 20th European White Dwarf Workshop, 20th European White Dwarf Workshop, Jul 2016, University of Warwick, Coventry, West Midlands, United Kingdom, United Kingdom. pp.355
Accession number :: edsair.dedup.wf.001..ebb1feb9beede4922b091e42ca859410

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