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Light Curve Analysis of Long Period Pulsating Stars with the Wavelet Method: The semiregular star V Boo

Published online by Cambridge University Press:  12 April 2016

K. Szatmáry ,
J. Gál  and
L. L. Kiss
K. Szatmáry
Affiliation:
Astron. Obs. and Dept. of Exp. Physics, JATE University, Dóm tér 9, H-6720, Szeged, Hungary, e-mail:K.Szatmary@physx.u-szeged.hu
J. Gál
Affiliation:
Astron. Obs. and Dept. of Exp. Physics, JATE University, Dóm tér 9, H-6720, Szeged, Hungary, e-mail:K.Szatmary@physx.u-szeged.hu
L. L. Kiss
Affiliation:
Astron. Obs. and Dept. of Exp. Physics, JATE University, Dóm tér 9, H-6720, Szeged, Hungary, e-mail:K.Szatmary@physx.u-szeged.hu

Abstract

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We have collected long data series of some SR and Mira stars from data banks. In many cases the light curves show strong fluctuation or variation in the period, phase and amplitude. The detection of the significant changes of these parameters is important from the point of view of pulsation theory and stellar evolution. We present here the analysis of V Boo. The used method is the Fourier and wavelet analysis in order to point out the modulations in the frequency and amplitude.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 417 - 418
Copyright
Copyright © Astronomical Society of the Pacific 1995