Towards Ensemble Asteroseismology of the Young Open Clusters Chi Persei and Ngc 6910

dc.contributor.author Saesen, S.
dc.contributor.author Pigulski, A.
dc.contributor.author Carrier, F.
dc.contributor.author Michalska, G.
dc.contributor.author Aerts, C.
dc.contributor.author De Ridder, J.
dc.contributor.author Zima, W.
dc.coverage.doi 10.1002/asna.201011462
dc.date.accessioned 2021-01-24T18:31:56Z
dc.date.available 2021-01-24T18:31:56Z
dc.date.issued 2010
dc.description 4th HELAS International Conference en_US
dc.description.abstract As 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, Weinheim en_US
dc.description.sponsorship Austrian Science Fund (FWF)Austrian Science Fund (FWF) [P 21830] Funding Source: researchfish en_US
dc.identifier.doi 10.1002/asna.201011462 en_US
dc.identifier.doi 10.1002/asna.201011462
dc.identifier.issn 0004-6337
dc.identifier.issn 1521-3994
dc.identifier.scopus 2-s2.0-78649410666
dc.identifier.uri https://doi.org/10.1002/asna.201011462
dc.identifier.uri https://hdl.handle.net/11147/10008
dc.language.iso en en_US
dc.publisher John Wiley and Sons Inc. en_US
dc.relation.ispartof Astronomische Nachrichten en_US
dc.rights info:eu-repo/semantics/closedAccess en_US
dc.subject techniques: photometric en_US
dc.subject stars: oscillations en_US
dc.subject open clusters and associations: individual (chi Per, NGC 6910) en_US
dc.title Towards Ensemble Asteroseismology of the Young Open Clusters Chi Persei and Ngc 6910 en_US
dc.type Conference Object en_US
dspace.entity.type Publication
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gdc.description.department İzmir Institute of Technology. Physics en_US
gdc.description.departmenttemp [Saesen, S.; Carrier, F.; Aerts, C.; De Ridder, J.; Briquet, M.; Acke, B.; Bauwens, E.; Beck, P. G.; Blom, Y.; Blommaert, J.; Broeders, E.; Davignon, G.; Debosscher, J.; Degroote, P.; Decin, L.; Dehaes, S.; De Meester, W.; Deroo, P.; Desmet, M.; Drummond, R.; Gielen, C.; Huygen, R.; Ladjal, D.; Lefever, K.; Ostensen, R.; Prins, S.; Antolin, E. Puga; Raskin, G.; Reyniers, M.; Vanautgaerden, J.; Vandenbussche, B.; Van Helshoecht, V.; Vanhollebeke, E.; Van Winckel, H.; Verhoelst, T.; Vuckovic, M.; Waelkens, C.; Yakut, K.; Zima, W.] Katholieke Univ Leuven, Inst Sterrenkunde, Leuven, Belgium; [Pigulski, A.; Michalska, G.; Kolaczkowski, Z.; Kopacki, G.; Narwid, A.; Steslicki, M.] Uniwersytetu Wroclawskiego, Inst Astron, Wroclaw, Poland; [Handler, G.; Beck, P. G.; Le en_US
gdc.description.endpage 1083 en_US
gdc.description.issue 09.Oct en_US
gdc.description.publicationcategory Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı en_US
gdc.description.scopusquality Q3
gdc.description.startpage 1080 en_US
gdc.description.volume 331 en_US
gdc.description.wosquality Q3
gdc.identifier.openalex W2095439184
gdc.identifier.wos WOS:000285211700046
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gdc.oaire.keywords techniques: photometric
gdc.oaire.keywords Astrophysics - Solar and Stellar Astrophysics
gdc.oaire.keywords Stars: oscillations
gdc.oaire.keywords FOS: Physical sciences
gdc.oaire.keywords Open clusters and associations: individual (? Per, NGC 6910)
gdc.oaire.keywords stars: oscillations
gdc.oaire.keywords Techniques: photometric
gdc.oaire.keywords Solar and Stellar Astrophysics (astro-ph.SR)
gdc.oaire.keywords open clusters and associations: individual (chi Per, NGC 6910)
gdc.oaire.popularity 6.1791405E-10
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gdc.oaire.sciencefields 0103 physical sciences
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