The null result of a search for pulsational variations of the surface magnetic field in the roAp star γ Equulei
- Author
- 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 - Source
Monthly Notices of the Royal Astronomical Society. 2004, Vol 351, Num 2, pp L34-L38 ; ref : 16 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- Russian
- Author keyword
- stars: chemically peculiar stars: individual: y Equ stars: magnetic fields stars: oscillations
- Keyword (fr)
- Borne supérieure Champ magnétique Etoile Ap Etoile chimiquement particulière Série temporelle
- Keyword (en)
- Upper bound Magnetic fields Ap stars Chemically peculiar star Time series
- Keyword (es)
- Cota superior Estrella quimicamente particular
- Classification
- 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.)
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 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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DOI
10.1111/j.1365-2966.2004.07946.x 
https://dx.doi.org/10.1111/j.1365-2966.2004.07946.x
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