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SMEI observations of previously unseen pulsation frequencies in γ Doradus

Tarrant, N.J and Chaplin, W.J and Elsworth, Y. P and Spreckley, S.A and Stevens, I.R (2008) SMEI observations of previously unseen pulsation frequencies in γ Doradus. Astronomy and Astrophysics, 492 (1). pp. 167-169. ISSN 0004-6361

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URL of Published Version: http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/pdf/2008/46/aa10952-08.pdf

Identification Number/DOI: 10.1051/0004-6361:200810952

Aims. As g-mode pulsators, gamma-Doradus-class stars may naïvely be expected to show a large number of modes. Taking advantage of the long photometric time-series generated by the solar mass ejection imager (SMEI) instrument, we have studied the star gamma Doradus to determine whether any other modes than the three already known are present at observable amplitude.
Methods. High-precision photometric data from SMEI taken between April 2003 and March 2006 were subjected to periodogram analysis with the PERIOD04 package.
Results. We confidently determine three additional frequencies at 1.39, 1.87, and 2.743 d−1. These are above and beyond the known frequencies of 1.320, 1.364, and 1.47 d−1.
Conclusions. Two of the new frequencies, at 1.39 and 1.87 d−1, are speculated to be additional modes of oscillation, with the third frequency at 2.743−1 a possible combination frequency.

Type of Work:Article
Date:01 October 2008 (Publication)
School/Faculty:Colleges (2008 onwards) > College of Engineering & Physical Sciences
Department:School of Physics and Astronomy
Subjects:QB Astronomy
QC Physics
Institution:University of Birmingham
Copyright Holders:EDP Sciences
ID Code:380
Refereed:YES
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