A Study of Contact Binaries with Large Temperature Differences between Components
Abstract
We present an extensive analysis of new light and radial velocity (RV) curves, as well as high quality broadening function (BF) profiles of twelve binary systems for which a contact configuration with large temperature differences between components has been reported in the literature. We find that six systems (V1010 Oph, WZ Cyg, VV Cet, DO Cas, FS Lup, V747 Cen) have near contact configurations. For the remaining systems (CX Vir, FT Lup, BV Eri, FO Hya, CN And, BX And), our solutions of the new observations once again converge in a contact configuration with large temperature differences between the components. However, the bright regions discovered in the BFs for V747 Cen, CX Vir, FT Lup, BV Eri, FO Hya, and CN And, and further attributed to hot spots, shed new light on the physical processes taking place between the components and imply the possibility that the contact configurations obtained from light and RV curve modeling are a spurious result.
- Publication:
-
Acta Astronomica
- Pub Date:
- December 2010
- DOI:
- 10.48550/arXiv.1011.5682
- arXiv:
- arXiv:1011.5682
- Bibcode:
- 2010AcA....60..305S
- Keywords:
-
- binaries: eclipsing;
- binaries: close;
- Stars: fundamental parameters;
- Stars: individual: V1010 Oph;
- WZ Cyg;
- VV Cet;
- DO Cas;
- FS Lup;
- V747 Cen;
- CX Vir;
- FT Lup;
- BV Eri;
- FO Hya;
- CN And;
- BX And;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- Submited to Acta Astronomica