The EC 14026 stars – V. The pulsation periods of PB 8783 |
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| Authors: | O'Donoghue Koen Solheim Barstow Dobbie O'Brien Clemens Sullivan & Kawaler |
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| Institution: | Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa,;South African Astronomical Observatory, PO Box 9, Observatory 7935, Cape, South Africa,;Institutt for Matematiske Realfag, Universitet i Trømso, 9000 Trømso, Norway,;Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH,;Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA,;California Institute of Technology, Pasadena, CA 91125, USA,;Department of Physics, Victoria University, Box 600, Wellington, New Zealand |
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| Abstract: | PB 8783 is a member of the newly discovered class of pulsating sdB stars, the EC 14026 stars. The potential of the pulsations of these stars as diagnostic probes of their interiors can only be realized fully by intensive campaigns of multisite time series photometry. To this end we have undertaken a campaign spanning 2 weeks and involving data from five different sites. 183 h of data were obtained. Frequency analysis yielded at least 11 pulsation periods in seven discrete groups between 94 and 136 s. Three of the periods in one specific group are equally spaced in frequency, with a spacing of 0.94 μHz. The frequency spacings amongst the members of other groups are similar to this. A rotation period of ～12 d is implied. A general scheme for identifying the observed modes is suggested. The periods from a detailed model are in good overall agreement with the observed periods, but some difficulties remain. Three additional periods in the range 61–63 s, and with very low amplitude, were also found. No convincing interpretation of these could be devised. |
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| Keywords: | binaries: close stars: individual: PB 8783 stars: oscillations |
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