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dc.contributor.authorRodríguez, Eloy
dc.contributor.authorFauvaud, S.
dc.contributor.authorFarrell, J. A.
dc.contributor.authorZhou, A.-Y.
dc.contributor.authorSareyan, J.-P.
dc.contributor.authorLópez-González, M. J.
dc.contributor.authorDupret, M.-A.
dc.contributor.authorGrigahcéne, A.
dc.contributor.authorde Ridder, J.
dc.contributor.authorKlingenberg, G.
dc.contributor.authorWolf, Marek
dc.contributor.authorVan Cauteren, P.
dc.contributor.authorLampens, P.
dc.contributor.authorMartínez, D.
dc.contributor.authorCasanova, V. M.
dc.contributor.authorAceituno, F. J.
dc.contributor.authorHelvaci, M.
dc.contributor.authorHintz, E. G.
dc.contributor.authorKrál, Lukáš
dc.contributor.authorFumagalli, F.
dc.contributor.authorSimonetti, J. H.
dc.contributor.authorGranslo, B. H.
dc.contributor.authorKotková, Lenka
dc.contributor.authorSantacana, G.
dc.contributor.authorMichelet, J.
dc.contributor.authorFauvaud, M.
dc.contributor.authorVugnon, J.-M.
dc.contributor.authorSadsaoud, H.
dc.contributor.authorAliouane, A.
dc.contributor.authorGrigahcéne, Z. C.
dc.contributor.authorMartín-Ruíz, Susana
dc.contributor.authorAmado, Pedro José
dc.contributor.authorSuárez, Juan Carlos
dc.contributor.authorMoya, A.
dc.contributor.authorKučáková, Hana
dc.contributor.authorKocián, Radek
dc.contributor.authorTruparová, B.
dc.contributor.authorAvdibegović, A.
dc.contributor.authorBlažek, Martin
dc.contributor.authorKliner, J.
dc.contributor.authorZasche, Petr
dc.contributor.authorVilásek, M.
dc.contributor.authorBartošíková, S.
dc.contributor.authorYasarsoy, B.
dc.contributor.authorUlusoy, C.
dc.contributor.authorGraham, K. A.
dc.contributor.authorNicholson, M. P.
dc.contributor.authorTrondal, O.
dc.contributor.authorYesilyaprak, C.
dc.contributor.authorCoker, D.
dc.date.accessioned2018-03-26T09:12:57Z
dc.date.available2018-03-26T09:12:57Z
dc.date.issued2007
dc.identifier.citationAstronomy & Astrophysics. 2007, vol. 471, issue 1, p. 255-264.cs
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/10084/125347
dc.description.abstractContext. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very complex frequency spectrum is detected, with a number of independent nonradial modes excited, unusual among the high-amplitude pulsators in the Lower Classical Instability Strip. Aims. An extensive and detailed study has been carried out to investigate the pulsational content and properties of this object. Methods. The analysis is based on 283 h of CCD observations obtained in the Johnson V filter, during a long multisite photometric campaign carried out along the Northern autumn-winter of 2005-2006. Additionally, multicolour BI photometry was also collected to study the phase shifts and amplitude ratios, between light curves obtained in different filters, for modal discrimination of the main excited modes. Results. The detailed frequency analysis revealed a very rich and dense pulsational content consisting of 25 significant peaks, 22 of them corresponding to independent modes: one is the already known main periodicity f(0) = 25.5765 cd(-1) (Delta V = 153 mmag) and the other 21 are excited modes showing very small amplitudes. Some additional periodicities are probably still remaining in the residuals. This represents the most complex spectrum ever detected in a high-amplitude pulsator of this type. The majority of the secondary modes suspected from earlier works are confirmed here and, additionally, a large number of new peaks are detected. The amplitude of the main periodicity f(0) seems to be stable during decades, but the majority of the secondary modes show strong amplitude changes from one epoch to another. The suspected fundamental radial nature of the main periodicity of BL Cam is confirmed, while the secondary peak f(1) = 25.2523 cd(-1) is identified as a nonradial mixed mode g(4) with l = 1. The radial double-mode nature, claimed by some authors for the main two frequencies of BL Cam, is not confirmed. Nevertheless, the frequency f(6) = 32.6464 cd(-1) could correspond to the first radial overtone.cs
dc.language.isoencs
dc.publisherEDP Sciencescs
dc.relation.ispartofseriesAstronomy & Astrophysicscs
dc.relation.urihttps://doi.org/10.1051/0004-6361:20077514cs
dc.rights© ESO 2007cs
dc.subjectstars: variables: δ Sctcs
dc.subjectstars: individual: BL Camelopardaliscs
dc.subjectstars: oscillationscs
dc.subjecttechniques: photometriccs
dc.titleThe field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign - I. Pulsationcs
dc.typearticlecs
dc.identifier.doi10.1051/0004-6361:20077514
dc.type.statusPeer-reviewedcs
dc.description.sourceWeb of Sciencecs
dc.description.volume471cs
dc.description.issue1cs
dc.description.lastpage264cs
dc.description.firstpage255cs
dc.identifier.wos000248394400032


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