WAVELET ANALYSIS OF 173 SEMI-REGULAR VARIABLES
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Дата
2010
Автори
Науковий керівник
Укладач
Редактор
Назва журналу
ISSN
E-ISSN
Назва тому
Видавець
Astroprint
Анотація
We made the wavelet analysis of 173 semi-regular pulsating variable stars of di erent
sub-types. For the analysis, we have used 1,000,000 individual brightness estimates from the published international databases of the VSOLJ (Japan) and AFOEV (France). They were visually checked using the program OL (I.L.Andronov, 2001OAP....14..255A), and bad points were removed from the data les. The
wavelet analysis was performed using the program WWZ (I.L.Andronov, 1998KFNT...14..490A) which improves the discrete Morlet-type wavelet transform
to the case of irregularly spaced data. Mean weighted wavelet periodograms are presented, as well as wavelet maps. Dependences of the wavelet-based periods and amplitudes on time are presented for the investigated stars. Some stars exhibit switchings between preferred periods, which are interpreted as switchings of the pulsation mode. Additional criteria for classi cation of the pulsating variables based on the stability of periods and amplitudes are discussed. Results are
shown for the semi-regular star RU And, for which the semi-amplitude varies drastically from 0.027 (\nearly constant star") to 1.204 mag (\Mira"- type pulsating variable. The phase of pulsations also varies drastically by 0.7P, and the wavelet estimates of the
period - from 210 to 270 days.
Опис
Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 07/2010 . – Vol.23.
Ключові слова
Variable stars: pulsating: Semi- Regular: RU And, Data analysis
Бібліографічний опис
Odessa Astronomical Publications