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The null result of a search for pulsational variations of the surface magnetic field in the roAp star γ Equulei

Autor
KOCHUKHOV, O1 ; RYABCHIKOVA, T1 2 ; LANDSTREET, J. D3 ; WEISS, W. W1
[1] Department of Astronomy, University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
[2] Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya 48, 119017 Moscow, Russian Federation
[3] Department of Physics and Astronomy, University of Western Ontario, London, Ontario N6A 3K7, Canada
Fuente

Monthly Notices of the Royal Astronomical Society. 2004, Vol 351, Num 2, pp L34-L38 ; ref : 16 ref

CODEN
MNRAA4
ISSN
0035-8711
Campo Científico
Astronomy earth cosmic environment
Editor
Blackwell Science, Oxford
País de la publicación
United Kingdom
Tipo de documento
Article
Idioma
Russian
Palabra clave de autor
stars: chemically peculiar stars: individual: y Equ stars: magnetic fields stars: oscillations
Palabra clave (fr)
Borne supérieure Champ magnétique Etoile Ap Etoile chimiquement particulière Série temporelle
Palabra clave (in)
Upper bound Magnetic fields Ap stars Chemically peculiar star Time series
Palabra clave (es)
Cota superior Estrella quimicamente particular
Clasificación
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10L Magnetic and electric fields. Polarization of starlight

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C30 Variable and peculiar stars (including novae) / 001E03C30F Chemically peculiar stars (ap, am, etc.)

Disciplina
Astronomy
Procedencia
Inist-CNRS
Base de datos
PASCAL
Identificador INIST
15864926

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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