The rapidly oscillating Ap star HD 99563 and its distorted dipole pulsation mode
- Author
- HANDLER, G1 2 ; WEISS, W. W1 ; GARRIDO, R8 ; MEDUPE, R2 ; SHOBBROOK, R. R3 ; PAUNZEN, E1 ; HEMPEL, A4 ; ANGUMA, S. K5 ; KALEBWE, P. C6 ; KILKENNY, D2 ; MARTINEZ, P2 ; MOALUSI, M. B7
[1] Institut für Astronomie, Universität Wien, Türkenschanzstraβe 17, 1180 Wien, Austria
[2] South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa
[3] Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT, Australia
[4] Observatoire de Genève, Chemin des Maillettes 51, 1290 Sauverny, Switzerland
[5] Department of Physics, Mbarara University of Science and Technology, PO Box 1410, Mbarara, Uganda
[6] Physics Department, The University of Zambia, PO Box 32379, Lusaka, Zambia
[7] Department of Physics, University of the North-West, Private Bag X2046, Mmabatho 2735, South Africa
[8] Instituto de Astrofisica de Andalucia, Apt. 3044, 18080 Granada, Spain - Source
Monthly Notices of the Royal Astronomical Society. 2006, Vol 366, Num 1, pp 257-266, 10 p ; ref : 39 ref
- 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: individual: HD 99563 stars: individual: XY Crt stars: oscillations stars: variables: other techniques: photometric
- Keyword (fr)
- Bande instabilité Dipôle Etoile Ap Harmonique sphérique Mode oscillation Obliquité Pulsation stellaire Spectre stellaire Série temporelle
- Keyword (en)
- Instability strip Dipoles Ap stars Spherical harmonics Oscillation modes Obliqueness Stellar pulsations Stellar spectra Time series
- Keyword (es)
- Banda inestabilidad Oblicuidad
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17575485
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.1365-2966.2005.09849.x 
https://dx.doi.org/10.1111/j.1365-2966.2005.09849.x
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