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https://hdl.handle.net/11147/5056
Title: | The short-period low-mass binary system CC Com revisited | Authors: | Köse, O Kalomeni, Belinda Keskin, Varol Ulaş, Burak Yakut, Kadri |
Keywords: | Stars Binaries Eclipsing Evolutionary status |
Publisher: | John Wiley and Sons Inc. | Source: | 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 | 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. | URI: | https://doi.org/10.1002/asna.201011566 http://hdl.handle.net/11147/5056 |
ISSN: | 0004-6337 1521-3994 |
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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