An analysis of the light curves of the overcontact binary system V2388 Ophiuchi
Articles > Article · 2004
Authors: Kadri YAKUT, Belinda KALOMENİ YAKUT, C Ibanoglu
Astronomy & Astrophysics, Journal Indexed in SCI Expanded, International, WoS, 2004, vol 417, pp 725-730
DOI: 10.1051/0004-6361:20031773
Summary
We present four seasons' (2000–2003) ground-based photometry of the short-period contact binary V2388 Oph. The system is the brighter component of visual binary HIP 87655. The magnitude difference between the visual companion and the eclipsing pair was estimated to be , and in B, V and R bandpasses, respectively. The light curves in BVR are solved by the WD code. Combining the parameters found by the light curve analysis with those of the radial velocity solution we derived the masses and radii of the star components as: , , , . The primary component appears to be more evolved in the mass-radius, mass-luminosity planes and also in the HR diagram. It lies near the terminal-age main-sequence, which agrees well with the position of deeper-contact A-type systems. The large fill-out factor of 0.65 does also support this classification.