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20092021
most citedPhysical parameters of close binary systems: VIII

31 citations · 58 across the 11 of their papers we have counts for

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16 papers

astro-ph.SR202131 cited

Physical parameters of close binary systems: VIII

K. Gazeas, S. Zola, A. Liakos +13

This paper presents the results of a combined spectroscopic and photometric study of 20 contact binary systems: HV Aqr, OO Aql, FI Boo, TX Cnc, OT Cnc, EE Cet, RWCom, KR Com, V401…

astro-ph.SR2020

International observational campaign of the 2014 eclipse of EE Cep

D. Pieńkowski, C. Gałan, T. Tomov +64

Context. EE Cep is one of few eclipsing binary systems with a dark, dusty disk around an invisible object similar to ε Aur. The system is characterized by grey and asymmetric eclip…

astro-ph.SR2018

New light curve solution of V568 Peg and first determination of its fundamental parameters

Diana Kjurkchieva, Sunay Ibryamov

We present V, Rc photometric observations of the short-period W UMa star V568 Peg. They allowed us to improve its period. The light curve solution revealed that V568 Peg is an over…

astro-ph.IM2018

First observations with the 25 cm telescope of the Shumen Astronomical Observatory

Diana Kjurkchieva, Sunay Ibryamov, Borislav Borisov +3

The first observations with the 25 cm telescope of the Shumen Astronomical Observatory led to the following conclusions: (a) Intra-night observations of variable stars with an ampl…

astro-ph.SR2018

The W UMa binaries USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac: light curve solutions and global parameters based on the GAIA distances

Diana P. Kjurkchieva, Velimir A. Popov, Yordanka Eneva +1

We present photometric observations in Sloan filters g', i' of the eclipsing W UMa stars USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac. The sinusoidal-like O-C diagram o…

astro-ph.SR2018

NSVS 2569022: a peculiar binary among the W UMa stars with extremely small mass ratios

Diana P. Kjurkchieva, Velimir A. Popov, Nikola I. Petrov

Photometric observations of the W UMa binary NSVS 2569022 are presented. The light curve solution reveals that both components are of F spectral type (temperatures ==6100…