Towards ensemble asteroseismology of the young open clusters chi Persei and NGC 6910

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dc.contributor.authorSaesen, S.
dc.contributor.authorPigulski, A.
dc.contributor.authorCarrier, F.
dc.contributor.authorMichalska, G.
dc.contributor.authorAerts, C.
dc.contributor.authorDe Ridder, J.
dc.contributor.authorBriquet, M.
dc.contributor.authorHandler, G.
dc.contributor.authorKolaczkowski, Z.
dc.contributor.authorAcke, B.
dc.contributor.authorBauwens, E.
dc.contributor.authorBeck, P. G.
dc.contributor.authorBlom, Y.
dc.contributor.authorBlommaert, J.
dc.contributor.authorBroeders, E.
dc.contributor.authorCherix, M.
dc.contributor.authorDavignon, G.
dc.contributor.authorDebosscher, J.
dc.contributor.authorDegroote, P.
dc.contributor.authorDecin, L.
dc.contributor.authorDehaes, S.
dc.contributor.authorDe Meester, W.
dc.contributor.authorDeroo, P.
dc.contributor.authorDesmet, M.
dc.contributor.authorDrummond, R.
dc.contributor.authorEggen, J. R.
dc.contributor.authorFu, J.
dc.contributor.authorGazeas, K.
dc.contributor.authorGelven, G. A.
dc.contributor.authorGielen, C.
dc.contributor.authorHuygen, R.
dc.contributor.authorJiang, X.
dc.contributor.authorKalomeni, B.
dc.contributor.authorKim, S. -L.
dc.contributor.authorKim, D. H.
dc.contributor.authorKopacki, G.
dc.contributor.authorKwon, J. -H.
dc.contributor.authorLadjal, D.
dc.contributor.authorLee, C. -U.
dc.contributor.authorLee, Y. -J.
dc.contributor.authorLefever, K.
dc.contributor.authorLeitner, A.
dc.contributor.authorLenz, P.
dc.contributor.authorLiakos, A.
dc.contributor.authorLorenz, D.
dc.contributor.authorNarwid, A.
dc.contributor.authorNiarchos, P.
dc.contributor.authorOstensen, R.
dc.contributor.authorPoretti, E.
dc.contributor.authorPrins, S.
dc.contributor.authorProvencal, J.
dc.contributor.authorAntolin, E. Puga
dc.contributor.authorPuschnig, J.
dc.contributor.authorRaskin, G.
dc.contributor.authorReed, M. D.
dc.contributor.authorReyniers, M.
dc.contributor.authorSchmidt, E.
dc.contributor.authorSchmitzberger, L.
dc.contributor.authorSpano, M.
dc.contributor.authorSteininger, B.
dc.contributor.authorSteslicki, M.
dc.contributor.authorUytterhoeven, K.
dc.contributor.authorVanautgaerden, J.
dc.contributor.authorVandenbussche, B.
dc.contributor.authorVan Helshoecht, V.
dc.contributor.authorVanhollebeke, E.
dc.contributor.authorVan Winckel, H.
dc.contributor.authorVerhoelst, T.
dc.contributor.authorVuckovic, M.
dc.contributor.authorWaelkens, C.
dc.contributor.authorWolf, G. W.
dc.contributor.authorYakut, K.
dc.contributor.authorZhang, C.
dc.contributor.authorZima, W.
dc.date.accessioned2019-10-27T21:29:01Z
dc.date.available2019-10-27T21:29:01Z
dc.date.issued2010
dc.departmentEge Üniversitesien_US
dc.description4th HELAS International Conference -- FEB 01-05, 2010 -- Canary Islands, SPAINen_US
dc.description.abstractAs a result of the variability survey in chi Persei and NGC 6910, the number of beta Cep stars that are members of these two open clusters is increased to twenty stars, nine in NGC 6910 and eleven in chi Persei. We compare pulsational properties, in particular the frequency spectra, of beta Cep stars in both clusters and explain the differences in terms of the global parameters of the clusters. We also indicate that the more complicated pattern of the variability among B-type stars in chi Persei is very likely caused by higher rotational velocities of stars in this cluster. We conclude that the sample of pulsating stars in the two open clusters constitutes a very good starting point for the ensemble asteroseismology of beta Cep-type stars and maybe also for other B-type pulsators. (C) 2010 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheimen_US
dc.identifier.doi10.1002/asna.201011462
dc.identifier.endpage1083en_US
dc.identifier.issn0004-6337
dc.identifier.issn1521-3994
dc.identifier.issn0004-6337en_US
dc.identifier.issn1521-3994en_US
dc.identifier.issue09.Octen_US
dc.identifier.startpage1080en_US
dc.identifier.urihttps://doi.org/10.1002/asna.201011462
dc.identifier.urihttps://hdl.handle.net/11454/45242
dc.identifier.volume331en_US
dc.identifier.wosWOS:000285211700046en_US
dc.identifier.wosqualityQ3en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.language.isoenen_US
dc.publisherWiley-V C H Verlag Gmbhen_US
dc.relation.ispartofAstronomische Nachrichtenen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjecttechniques: photometricen_US
dc.subjectstars: oscillationsen_US
dc.subjectopen clusters and associations: individual (chi Per, NGC 6910)en_US
dc.titleTowards ensemble asteroseismology of the young open clusters chi Persei and NGC 6910en_US
dc.typeArticleen_US

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