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https://hdl.handle.net/11147/5056
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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Köse, O | - |
dc.contributor.author | Kalomeni, Belinda | - |
dc.contributor.author | Keskin, Varol | - |
dc.contributor.author | Ulaş, Burak | - |
dc.contributor.author | Yakut, Kadri | - |
dc.date.accessioned | 2017-03-15T07:17:04Z | - |
dc.date.available | 2017-03-15T07:17:04Z | - |
dc.date.issued | 2011-07 | - |
dc.identifier.citation | Köse, O., Kalomeni, B., Keskin, V., Ulaş, B., and Yakut, K. (2011). The short-period low-mass binary system CC Com revisited. Astronomische Nachrichten, 332(6), 626-630. doi:10.1002/asna.201011566 | en_US |
dc.identifier.issn | 0004-6337 | - |
dc.identifier.issn | 1521-3994 | - |
dc.identifier.uri | https://doi.org/10.1002/asna.201011566 | - |
dc.identifier.uri | http://hdl.handle.net/11147/5056 | - |
dc.description.abstract | In this study we determined precise orbital and physical parameters of the very short-period low-mass contact binary system CC Com. The parameters are obtained by analysis of new CCD data combined with archival spectroscopic data. The physical parameters of the cool and hot components are derived as Mc = 0.717(14) M⊙, Mh = 0.378(8) M⊙, Rc = 0.708(12) R⊙, Rh = 0.530(10) R⊙, Lc = 0.138(12) L⊙, and Lh = 0.085(7) L⊙, respectively, and the distance of the system is estimated as 64(4) pc. The times of minima obtained in this study and with those published before enable us to calculate the mass transfer rate between the components which is 1.6 × 10-8 M⊙ yr-1. Finally, we discuss the possible evolutionary scenario of CC Com. | en_US |
dc.description.sponsorship | Turkish Scientific and Research Council (TUBITAK 109T047); TUBITAK National Observatory (TUG); Ege University; Turkish Academy of Sciences (TUBA) | en_US |
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/openAccess | en_US |
dc.subject | Stars | en_US |
dc.subject | Binaries | en_US |
dc.subject | Eclipsing | en_US |
dc.subject | Evolutionary status | en_US |
dc.title | The short-period low-mass binary system CC Com revisited | en_US |
dc.type | Article | en_US |
dc.authorid | TR17457 | en_US |
dc.institutionauthor | Kalomeni, Belinda | - |
dc.department | İzmir Institute of Technology. Physics | en_US |
dc.identifier.volume | 332 | en_US |
dc.identifier.issue | 6 | en_US |
dc.identifier.startpage | 626 | en_US |
dc.identifier.endpage | 630 | en_US |
dc.identifier.wos | WOS:000293271400008 | en_US |
dc.identifier.scopus | 2-s2.0-79960253835 | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.identifier.doi | 10.1002/asna.201011566 | - |
dc.relation.doi | 10.1002/asna.201011566 | en_US |
dc.coverage.doi | 10.1002/asna.201011566 | en_US |
dc.identifier.wosquality | Q4 | - |
dc.identifier.scopusquality | Q3 | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
Appears in Collections: | Physics / Fizik Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection WoS İndeksli Yayınlar Koleksiyonu / WoS Indexed Publications Collection |
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