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KIC 6761539, a fast rotating γ Dor – δ Sct hybrid star

Published online by Cambridge University Press:  18 February 2014

W. Herzberg ,
D. Corre ,
K. Uytterhoeven  and
M. Roth
W. Herzberg
Affiliation:
Kiepenheuer-Institut für Sonnenphysik, 79104 Freiburg, Germany email: [email protected]
D. Corre
Affiliation:
Kiepenheuer-Institut für Sonnenphysik, 79104 Freiburg, Germany email: [email protected]
K. Uytterhoeven
Affiliation:
Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, 38200 La Laguna, Tenerife, Spain
M. Roth
Affiliation:
Kiepenheuer-Institut für Sonnenphysik, 79104 Freiburg, Germany email: [email protected]
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Abstract

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KIC 6761539 is one of many fast rotating γ Doradus – δ Scuti hybrid pulsators. A search for possible regularities in the frequency spectrum is performed and a first stellar model is presented.

Keywords

stars: individual KIC 6761539stars: oscillationsstars: variables: δ Scuti
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 419 - 420
Copyright
Copyright © International Astronomical Union 2014 

References

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Paxton, B., Bildsten, L., Dotter, A., Herwig, F., Lesaffre, P., & Timmes, F. 2011, ApJS, 192, 3CrossRefGoogle Scholar
Uytterhoeven, K., Moya, A., Grigahcène, A., et al. 2011, A&A, 534, A125Google Scholar