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2005 Photometric observations and multiple frequencies of the δ Scuti variable V350 Peg

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Abstract

We present the V light curves of δ Scuti type variable V350 Peg, obtained between August and October 2005 at the Ankara University Observatory (AUG) and the TÜBÍTAK National Observatory (TUG). By application of multiple-frequency analyses using Period04 to 7878 photometric V measurements (which are consist of our 747 V data and 7131 V data obtained at Monegrillo Observatory) of V350 Peg, a five-frequency solution was found to be fitted well to the data. In accordance with the computed Q values for V350 Peg, it was found that this star has probably radial mode with l=0 and g-mode oscillations.

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Authors and Affiliations

  1. Faculty of Science, Ankara University, 06100, Tandoğan, Ankara, Turkey

    F. Ekmekçi & S. Topal

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  1. F. Ekmekçi
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  2. S. Topal
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Correspondence to F. Ekmekçi.

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Ekmekçi, F., Topal, S. 2005 Photometric observations and multiple frequencies of the δ Scuti variable V350 Peg. Astrophys Space Sci 321, 101–107 (2009). https://doi.org/10.1007/s10509-009-0019-5

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  • DOI: https://doi.org/10.1007/s10509-009-0019-5

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