dc.contributor.author | Mikulášek, Zdeněk | |
dc.contributor.author | Gráf, Tomáš | |
dc.contributor.author | Krtička, Jiří | |
dc.contributor.author | Zverko, Juraj | |
dc.contributor.author | Žižňovský, Jozef | |
dc.date.accessioned | 2008-07-16T10:26:03Z | |
dc.date.available | 2008-07-16T10:26:03Z | |
dc.date.issued | 2008 | |
dc.identifier.citation | Contributions of the Astronomical Observatory Skalnaté Pleso. 2008. vol. 38, no. 2, p. 363-368. | en |
dc.identifier.issn | 1335-1842 | |
dc.identifier.issn | 1336-0337 | |
dc.identifier.uri | http://hdl.handle.net/10084/65877 | |
dc.description.abstract | We 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.iso | en | en |
dc.publisher | Astronomický ústav Slovenskej akadémie vied | en |
dc.relation.ispartofseries | Contributions of the Astronomical Observatory Skalnaté Pleso | en |
dc.relation.uri | http://www.ta3.sk/caosp/Eedition/FullTexts/vol38no2/pp363-368.pdf | en |
dc.subject | stars: chemically peculiar | en |
dc.subject | stars: variables: light curves | en |
dc.subject | methods: data analysis | en |
dc.title | mCP stars with photometrically simple
behaviour | en |
dc.type | article | en |
dc.identifier.location | Není ve fondu ÚK | en |
dc.identifier.wos | 000256514000040 | |