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Preliminary analysis of V and Hp light curves of 26 carbon Miras

dc.contributor.authorMikulášek, Zdeněk
dc.contributor.authorGráf, Tomáš
dc.date.accessioned2007-09-12T06:21:17Z
dc.date.available2007-09-12T06:21:17Z
dc.date.issued2005
dc.identifier.citationAstrophysics and Space Science. 2005, vol. 296, no. 1-4, p. 157-160.en
dc.identifier.issn0004-640X
dc.identifier.issn1572-946X
dc.identifier.urihttp://hdl.handle.net/10084/62694
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Scienceen
dc.relation.urihttps://doi.org/10.1007/s10509-005-4424-0en
dc.subjectephemerisen
dc.subjectcarbon starsen
dc.subjectcarbon Mirasen
dc.titlePreliminary analysis of V and Hp light curves of 26 carbon Mirasen
dc.typearticleen
dc.identifier.locationNení ve fondu ÚKen
dc.description.abstract-enLight variations of a representative sample of 26 more or less periodically variable carbon stars were analyzed on the basis of 2220 individual observations made by the Hipparcos satellite and 33 544 visual observations listed in AFOEV and VSOLJ databases within the interval JD = 2 448 000 (1988) ±6 cycles. We found the osculating linear ephemerides of all stars and their mean light curves, as well. We found that the light curves of the carbon Miras in our set can be satisfactorily expressed as a linear combination of only two basic light curves. The analysis was done by an own method combining robust regression and principal component analysis.en
dc.identifier.doi10.1007/s10509-005-4424-0
dc.identifier.wos000228820000020


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