23 citations · 41 across the 3 of their papers we have counts for
5 papers
Structure of accretion flows in the nova-like cataclysmic variable RW Tri
G. Subebekova, S. Zharikov, G. Tovmassian +5
We obtained photometric observations of the nova-like cataclysmic variable RW Tri and gathered all available AAVSO and other data from the literature. We determined the system para…
Properties of Galactic B[e] Supergiants: V. 3 Pup -- constraining the orbital parameters and modeling the circumstellar environments
A. S. Miroshnichenko, S. Danford, S. V. Zharikov +9
We report the results of a long-term spectroscopic monitoring of the A-type supergiant with the B[e] phenomenon 3 Pup = HD 62623. We confirm earlier findings that it is a binary sy…
IRAS 22150+6109 - a young B-type star with a large disc
Olga V. Zakhozhay, Anatoly S. Miroshnichenko, Kenesken S. Kuratov +4
We present the results of a spectroscopic analysis and spectral energy distribution (SED) modelling of the optical counterpart of the infrared source IRAS 22150+6109. The source wa…
Toward Understanding the B[e] Phenomenon. VII. AS 386, a single-lined binary with a candidate black hole component
S. A. Khokhlov, A. S. Miroshnichenko, S. V. Zharikov +24
We report the results of spectroscopic and photometric observations of the emission-line object AS 386. For the first time, we found that it exhibits the B[e] phenomenon and fits t…
Nonlinear fractal meaning of the Hubble constant
Zeinulla Zhanabaev, Serik Khokhlov, Aldiyar Agishev
According to astrophysical observations value of recession velocity in a certain point is proportional to a distance to this point. The proportionality coefficient is the Hubble co…