activity
19972025
most citedOptical photometry of the PSR B0656+14 and its neighborhood

56 citations · 1k across the 70 of their papers we have counts for

collaborators

70 papers

astro-ph.SR2025★ 1 cited

Dynamical Masses and Radiative Transfer Modeling of HD 698: a Be Binary in Evolutionary Transition

Ilfa A. Gabitova, Alex C. Carciofi, Tajan H. de Amorim +13

We present a detailed analysis of the early post-mass-transfer binary HD 698 (V742 Cas) combining high-resolution optical spectroscopy, long-baseline interferometry, and radiative-…

astro-ph.SR2025

The B[e] Phenomenon in Supergiants. A Result of Mass Transfer in Binaries, Mergers, or What?

Anatoly S. Miroshnichenko, Sergey V. Zharikov, Nadezhda L. Vaidman +1

The B[e] phenomenon discovered nearly 50 years ago features the presence of forbidden emission lines due to extended and dense circumstellar gas and large IR excesses due to the ra…

astro-ph.SR2024★ 10 cited

Investigation of the Nature of the B[e] Star CI Cam in the Optical Range

E. A. Barsukova, A. N. Burenkov, V. P. Goranskij +10

We report the results of 24 years of photometric and spectroscopic monitoring of CI Cam since its outburst in 1998. In the early years of our research, we identified a system compo…

astro-ph.SR2023★ 1 cited

Optical spectral observations of three binary millisecond pulsars

A. V. Bobakov, A. V. Karpova, S. V. Zharikov +3

We present the results of optical spectroscopy of stellar companions to three binary millisecond pulsars, PSRs J06212514, J23171439 and J23024442, obtained with the Gran T…

astro-ph.SR2023★ 7 cited

The Z Camelopardalis-type star AY Piscium: stellar and accretion disk parameters

Jan Kára, Sergey Zharikov, Marek Wolf +5

We present a new study of the Z~Cam-type eclipsing cataclysmic variable AY~Piscium with the aim of determining the fundamental parameters of the system and the structure of the acc…

astro-ph.SR2023

Revisiting FS Aurigae and its triple cataclysmic variable system hypothesis

Carlos E. Chavez, Andres Aviles, Nikolaos Georgakarakos +4

A very long term variability (VLPP), with period of 875 days, was observed in the long-term light curve of FS Aurigae in 2011. This periodicity was calculated on 6 cycles. We re-ex…