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A search for rapid pulsations among nine luminous Ap stars

Author
FREYHAMMER, L. M1 ; KURTZ, D. W1 ; CUNHA, M. S2 ; MATHYS, G3 ; ELKIN, V. G1 ; RILEY, J. D1
[1] Centre for Astrophysics, University of Central Lancashire, Preston PR1 2HE, United Kingdom
[2] Centro de Astrofisica da Universidade do Porto, Rua das Estrelas, 4150 Porto, Portugal
[3] European Southern Observatory, Casilla 19001, Santiago, Chile
Source

Monthly Notices of the Royal Astronomical Society. 2008, Vol 385, Num 3, pp 1402-1430, 29 p ; ref : 3/4 p

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Blackwell Science, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
stars: magnetic fields stars: oscillations stars: variables: other
Keyword (fr)
Bande instabilité Borne supérieure Champ intense Champ magnétique Convection Corrélation croisée Diagramme magnitude couleur Diffusion(transport) Elément chimique Etoile Ap Etoile magnétique Etoile séquence principale Ionisation Opacité Spectrométrie Structure atmosphérique Structure stellaire Vitesse radiale
Keyword (en)
Instability strip Upper bound High field Magnetic fields Convection Cross correlations Color-magnitude diagrams Diffusion Elements (chemical) Ap stars Magnetic stars Main sequence stars Ionization Opacity Spectroscopy Atmospheric structure Stellar structure Radial velocity
Keyword (es)
Banda inestabilidad Cota superior
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20235369

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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