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dc.contributor.authorMikulášek, Zdeněk
dc.contributor.authorGráf, Tomáš
dc.contributor.authorKrtička, Jiří
dc.contributor.authorZverko, Juraj
dc.contributor.authorŽižňovský, Jozef
dc.date.accessioned2008-07-16T10:26:03Z
dc.date.available2008-07-16T10:26:03Z
dc.date.issued2008
dc.identifier.citationContributions of the Astronomical Observatory Skalnaté Pleso. 2008. vol. 38, no. 2, p. 363-368.en
dc.identifier.issn1335-1842
dc.identifier.issn1336-0337
dc.identifier.urihttp://hdl.handle.net/10084/65877
dc.description.abstractWe analyzed ubvy and Hp light curves of 19 well-observed magnetic CP stars selected from the On-line Database of Photometric Observations of mCP Stars, of which light curves in all the five colours were similar.We assumed that among these stars with photometrically simple behaviour (PSB) could be found ones with a single photometric spot. The knowledge gained by analysing those simple situations would help us comprehend more complicated cases. Light curves of the 19 PSB mCP stars proved generally to be nearly symmetrical, but surprisingly diverse. The analysis shows that only in the case of HD110956B, HD188041, and perhaps HD193722 are we able to explain their photometric behaviour by a simple one-spot model. Occurrence of more than one photometric spot on an mCP star is therefore more typical.en
dc.language.isoenen
dc.publisherAstronomický ústav Slovenskej akadémie vieden
dc.relation.ispartofseriesContributions of the Astronomical Observatory Skalnaté Plesoen
dc.relation.urihttp://www.ta3.sk/caosp/Eedition/FullTexts/vol38no2/pp363-368.pdfen
dc.subjectstars: chemically peculiaren
dc.subjectstars: variables: light curvesen
dc.subjectmethods: data analysisen
dc.titlemCP stars with photometrically simple behaviouren
dc.typearticleen
dc.identifier.locationNení ve fondu ÚKen
dc.identifier.wos000256514000040


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