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Model atmosphere analysis of the weakly magnetic DZ white dwarf g165-7

Author
DUFOUR, P1 ; BERGERON, P1 ; SCHMIDT, G. D2 ; LIEBERT, James2 ; HARRIS, H. C3 ; KNAPP, G. R4 ; ANDERSON, S. F5 ; SCHNEIDER, D. P6
[1] Département de Physique, Université de Montréal, C.P. 6128, Succursale Centre-Ville, Montréal, PQ H3C 3J7, Canada
[2] Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States
[3] US Naval Observatory, P.O. Box 1149, Flagstaff, AZ 86002-1149, United States
[4] Princeton University Observatory, Peyton Hall, Princeton, NJ 08544, United States
[5] Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195, United States
[6] Department of Astronomy and Astrophysics, Pennsylvania State Univer sity, 525 Davey Laboratory, University Park, PA 16802, United States
Source

The Astrophysical journal. 2006, Vol 651, Num 2, pp 1112-1119, 8 p ; 1 ; ref : 47 ref

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
: stars: abundances stars: atmospheres stars: individual (G165-7) stars: magnetic fields white dwarfs
Keyword (fr)
Abondance stellaire Champ magnétique Etoile magnétique Modèle atmosphère Naine blanche
Keyword (en)
Stellar abundance Magnetic fields Magnetic stars Atmosphere model White dwarf stars
Keyword (es)
Abundancia estelar Modelo atmósfera
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18353933

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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