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Seismic investigation of the γ Dor star KIC 6462033: The first results of Kepler and ground-based follow up observations

Published online by Cambridge University Press:  18 February 2014

C. Ulusoy
Affiliation:
College of Graduate Studies, University of South Africa, PO Box 392, UNISA 0003, Pretoria, South Africa email: [email protected]
B. Ulaş
Affiliation:
Department of Astronomy and Space Sciences, Faculty of Sciences, University of Ege, Bornova, 35100, İzmir, Turkey
M. Damasso
Affiliation:
Astronomical Observatory of the Autonomous Region of the Aosta Valley (OAVdA) Loc. Lignan 39, 11020 Nus (Aosta), Italy Department of Physics and Astronomy, University of Padova, vicolo dell'Osservatorio 3, I-35122 Padova, Italy
A. Carbognani
Affiliation:
Astronomical Observatory of the Autonomous Region of the Aosta Valley (OAVdA) Loc. Lignan 39, 11020 Nus (Aosta), Italy
D. Cenadelli
Affiliation:
Astronomical Observatory of the Autonomous Region of the Aosta Valley (OAVdA) Loc. Lignan 39, 11020 Nus (Aosta), Italy
I. Stateva
Affiliation:
Institute of Astronomy with NAO, Bulgarian Academy of Sciences, blvd. Tsarigradsko chaussee 72, Sofia 1784, Bulgaria
I. Kh. Iliev
Affiliation:
Institute of Astronomy with NAO, Bulgarian Academy of Sciences, blvd. Tsarigradsko chaussee 72, Sofia 1784, Bulgaria
D. Dimitrov
Affiliation:
Institute of Astronomy with NAO, Bulgarian Academy of Sciences, blvd. Tsarigradsko chaussee 72, Sofia 1784, Bulgaria
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Abstract

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Preliminary results on the analysis of the Kepler light curve and photometric ground-based time series of γ Dor star KIC 6462033 (TYC 3144-646-1, V = 10.83, P = 0.69686 d) are presented in order to determine pulsation frequencies.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

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