Tuesday, June 28 SESSION 2 (contd.). Formation and Evolution of Close Binaries (Star + Star Systems and Planet + Star Systems) Chair: S. Rucinski
09:00 – 09:40 Small stars posing a big challenge: Eclipsing binaries with M-type components (I)
09:40 – 09:55 Orbital Period Decrease of Chromospherically Active Binaries (C)
09:55 – 10:10 Light-time effect in the eclipsing binaries GO Cyg, GW Cep, V505 Sgr, AR Aur (C)
DISCUSSION 20 min 10:30 – 11:00
POSTERS 2.1. X-ray Observations of Binary and Single Wolf-Rayet Stars with XMM- Newton and Chandra
2.2. Libration points in Schwarzschild’s circular restricted three-body problem
2.3. Symbiotic stars in the context of close binary evolution
2.4. CN Lyn: a triple lined spectroscopic system harbouring a close eclipsing binary
2.5. Properties of contact binaries inferred from a sample based on combined radial velocity and photometric solutions
2.6. On
2.7. Reliable detection of cyclic variations in O–C diagrams
2.8. Radiation Pressure and Surface Gravity of Close Binaries
2.9. Spacial distribution of W UMa – type stars
2.10. Modeling the 2004.5 brightening of the contact binary system V839 Oph
2.11. First photometric observations and preliminary results of binaries FO Aurigae, V1038 Herculis and V1039 Herculis
2.12. M onitoring possible light-time effect in the orbital period of some eclipsing binaries at the Ankara University observatory
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