The Short-Period Low-Mass Binary System Cc Com Revisited

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BRONZE

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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.

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Keywords

Stars, Binaries, Eclipsing, Evolutionary status, Evolutionary status, Binaries, Binaries: eclipsing, FOS: Physical sciences, Stars: individual (cc com), Stars, Stars: evolution, Astrophysics - Solar and Stellar Astrophysics, Binaries: close, Stars: low-mass, Eclipsing, Solar and Stellar Astrophysics (astro-ph.SR)

Fields of Science

01 natural sciences, 0103 physical sciences

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

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25

Volume

332

Issue

6

Start Page

626

End Page

630
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Scopus : 32

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