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Asteroseismology of the β Cephei star ν Eridani – I. Photometric observations and pulsational frequency analysis
Authors:G. Handler,R. R. Shobbrook &dagger  ,M. Jerzykiewicz,K. Krisciunas,T. Tshenye,E. Rodrí  guez,V. Costa,A.-Y. Zhou,R. Medupe,W. M. Phorah,R. Garrido,P. J. Amado,M. Paparó  ,D. Zsuffa,L. Ramokgali,R. Crowe,N. Purves,R. Avila,R. Knight,E. Brassfield,P. M. Kilmartin, P. L. Cottrell
Affiliation:Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17, A-1180 Wien, Austria;Australian National University, Canberra, ACT, Australia;Wroclaw University Observatory, ul. Kopernika 11, 51-622 Wroclaw, Poland;Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile;Las Campanas Observatory, Casilla 601, La Serena, Chile;Theoretical Astrophysics Programme, University of the North-West, Private Bag X2046, Mmabatho 2735, South Africa;Instituto de Astrofisica de Andalucia, C.S.I.C., Apdo. 3004, 18080 Granada, Spain;National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China;South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa;Konkoly Observatory, Box 67, H-1525 Budapest XII, Hungary;Department of Physics and Astronomy, University of Hawaii - Hilo, 200 West Kawili Street, Hilo, Hawaii, 96720-4091, USA;Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand
Abstract:
Keywords:techniques: photometric    stars: early-type    stars: individual: μ Eridani    stars: individual: ν Eridani    stars: oscillations    stars: variables: other
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