The enigmatic highly peculiar binary system HD 66051

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dc.bibliographicCitation.firstPage621eng
dc.bibliographicCitation.issue2eng
dc.bibliographicCitation.journalTitleContributions of the Astronomical Observatory Skalnate Pleso : CAOSPeng
dc.bibliographicCitation.lastPage623eng
dc.bibliographicCitation.volume50eng
dc.contributor.authorPaunzen, E.
dc.contributor.authorNiemczura, E.
dc.contributor.authorKolaczek-Szymanski, P.A.
dc.contributor.authorHubrig, S.
dc.date.accessioned2021-07-27T05:01:17Z
dc.date.available2021-07-27T05:01:17Z
dc.date.issued2020
dc.description.abstractHD 66051 (V414 Pup) is an eclipsing and spectroscopic double-lined binary, hosting two chemically peculiar stars: a highly peculiar B star as pri-mary and an Am star as secondary. It also shows out-of-eclipse variability that is due to chemical spots. Using a set of high-resolution spectropolarimetric observations, a weak magnetic field on the primary was found. The investigation of the new high-resolution UVES spectrum of HD 66051 allowed us to decide on the chemical peculiarity type of both components with more reliability. © 2020 Astronomical Institute, Slovak Academy of Sciences.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/6369
dc.identifier.urihttps://doi.org/10.34657/5416
dc.language.isoengeng
dc.publisherTatranská Lomnica : Astronomický Ústav SAVeng
dc.relation.doihttps://doi.org/10.31577/CAOSP.2020.50.2.621
dc.relation.essn1336-0337
dc.relation.issn0862-920X
dc.relation.issn1335-1842
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subject.ddc530eng
dc.subject.ddc520eng
dc.subject.otherBinaries: eclipsingeng
dc.titleThe enigmatic highly peculiar binary system HD 66051eng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorAIPeng
wgl.subjectPhysikeng
wgl.typeZeitschriftenartikeleng
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