MIRAS OR SRA’S – THE TRANSIENT TYPE VARIABLES

dc.contributor.authorMarsakova, V. I.
dc.contributor.authorAndronov, Ivan L.
dc.date.accessioned2014-03-16T09:03:29Z
dc.date.available2014-03-16T09:03:29Z
dc.date.issued2012
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2012 . – Vol.25/1.uk
dc.description.abstractThe variability of several stars shows “Mira-type” and “semiregular” behavior during long-time data ranges. Such data are available due to amateur visual observations from AAVSO and AFOEV databases. We have studied these properties by using different methods of timeseries analysis, such as the periodogram analysis using trigonometric polynomial fit, wavelet analysis and individual cycle characteristics analysis using the running parabola fit. As the result, very similar multiperiodicities were detected.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4662
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;vol. 25, issue 1, p. 60-63.
dc.subjectStars: LPVsuk
dc.subjectMira-typeuk
dc.subjectsemiregularuk
dc.subjectindividual: S Aql, S Tri, Y Peruk
dc.titleMIRAS OR SRA’S – THE TRANSIENT TYPE VARIABLESuk
dc.typeArticleuk
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