activity
20132020
most citedThird components with elliptical orbits in the eclipsing binaries

4 citations · 5 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2020

Third components with elliptical orbits in the eclipsing binaries: BD and, SV Cam, V0836 Cyg & XZ CMi

D. E. Tvardovskyi

This is our regular research in the field of cyclic O-C changes and third components. In this article the results of four new stars investigation is described. These stars are: BD…

astro-ph.SR2019★ 1 cited

Third components with elliptical orbits in the eclipsing binaries: EQ Tau, IR Cas, IV Cas, RY Aqr & RZ Com

D. E. Tvardovskyi

This research is our forth article related to the topic of cyclic O-C changes, third components as the physical process that cause these changes and elliptical orbits of the third…

astro-ph.SR2019★ 4 cited

Third components with elliptical orbits in the eclipsing binaries

D. E. Tvardovskyi, V. I. Marsakova, I. L. Andronov

In our research, we studied 9 eclipsing binary stars: AR Lac, U CrB, S Equ, SU Boo, VV UMa, WW Gem, YY Eri, V0404 Lyr, HP Aur. We collected large sets of moments of minima from BRN…

astro-ph.SR2019

Third components with elliptical orbits in the eclipsing binaries: AB Cas, AF Gem, AR Boo, BF Vir and CL Aur

Dmytro Tvardovskyi

In this research, five eclipsing binary stars were studied: AB Cas, AF Gem, AR Boo, BF Vir and CL Aur. The large sets of moments of minima were used: from the international BRNO da…

astro-ph.SR2014

Statistical Studies of Long - Period Variable Stars in Odessa

Larisa S. Kudashkina, Ivan L. Andronov, Vladislava I. Marsakova +1

The studies of pulsating variable stars are traditional subjects of astronomers in Odessa. In the last half of the 20th century, the studies of the physical variable stars were the…

astro-ph.SR2013

Miras or SRA'S - the Transient Type Variables

Vladislava I. Marsakova, Ivan L. Andronov

The group of Mira-type and semi-regular variables with similar periodicity (multiperiodicty) is analyzed. They have periods of 230-260 days and 140-150 days and show intervals of p…