Please use this identifier to cite or link to this item: 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
Issue Date: Jul-2011
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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