Rotation and oblique pulsation in Kepler observations of the roAp star KIC 10483436

Photometry of KIC 10483436 was obtained continuously with 1-min exposures over a 27-d period from the Kepler satellite. The light curve shows rotational variations from surface spots with a period of 4.303 ± 0.002 d, an amplitude of about 6 mmag and eight pulsation frequencies typical of roAp stars....

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2011-06, Vol.413 (4), p.2651-2657
Hauptverfasser:	Balona, L. A., Cunha, M. S., Gruberbauer, M., Kurtz, D. W., Saio, H., White, T. R., Christensen-Dalsgaard, J., Kjeldsen, H., Christiansen, J. L., Hall, J. R., Seader, S. E.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Space telescopes Stars & galaxies stars: chemically peculiar stars: individual: KIC 10483436 stars: oscillations
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