"Inter-Longitude Astronomy" project: long period variable stars

This article contains the highlights of complex studies of long-period variable stars such as Miras: semiregular, symbiotic (particularly, pulsating symbiotic), as well as RV Tauri-type stars. In the course of these studies, important characteristics of mean light curves were determined. In the case...

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Бібліографічні деталі
Дата:2014
Автори: Andronov, I.L., Marsakova, V.I., Kudashkina, L.S., Chinarova, L.L.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2014
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/119804
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:"Inter-Longitude Astronomy" project: long period variable stars / I.L. Andronov, V.I. Marsakova, L.S. Kudashkina, L.L. Chinarova // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 3-8. — Бібліогр.: 48 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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Резюме:This article contains the highlights of complex studies of long-period variable stars such as Miras: semiregular, symbiotic (particularly, pulsating symbiotic), as well as RV Tauri-type stars. In the course of these studies, important characteristics of mean light curves were determined. In the case of multi-component variability, additional periods were found. Correlations between parameters of mean light curves were investigated. The cycle-to-cycle changes of light curve parameters were analysed using various mathematical methods. Classification criteria of variable stars and effects of variability were proposed based on this research. The study of observational parameters and the correlations between them can be used to estimate the age, mass, and other physical characteristics of AGB stars.