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SuperWASP observations of pulsating Am stars

Smalley, B.; Kurtz, D. W.; Smith, A. M. S.; Fossati, L.; Anderson, D. R.; Barros, S. C. C.; Butters, O. W.; Collier Cameron, A.; Christian, D. J.; Enoch, B.; Faedi, F.; Haswell, C. A.; Hellier, C.; Holmes, S.; Horne, K.; Kane, S. R.; Lister, T. A.; Maxted, P. F. L.; Norton, A. J.; Parley, N.; Pollacco, D.; Simpson, E. K.; Skillen, I.; Southworth, J.; Street, R. A.; West, R. G.; Wheatley, P. J. and Wood, P. L. (2011). SuperWASP observations of pulsating Am stars. Astronomy & Astrophysics, 535, article no. A3.

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DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1051/0004-6361/201117230
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Abstract

We have studied over 1600 Am stars at a photometric precision of 1 mmag with SuperWASP photometric data. Contrary to previous belief, we find that around 200 Am stars are pulsating δ Sct and γ Dor stars, with low amplitudes that have been missed in previous, less extensive studies. While the amplitudes are generally low, the presence of pulsation in Am stars places a strong constraint on atmospheric convection, and may require the pulsation to be laminar. While some pulsating Am stars have been previously found to be δ Sct stars, the vast majority of Am stars known to pulsate are presented in this paper. They will form the basis of future statistical studies of pulsation in the presence of atomic diffusion.

Item Type: Journal Article
Copyright Holders: 2011 ESO
ISSN: 1432-0746
Extra Information: 32 pp
Keywords: asteroseismology; chemically peculiar stars; stellar oscillations; variable stars; delta Scuti; photometric techniques
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 29893
Depositing User: Andrew Norton
Date Deposited: 27 Oct 2011 15:50
Last Modified: 21 Jul 2014 18:45
URI: http://oro.open.ac.uk/id/eprint/29893
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