activity
19962024
most citedDust Emission from Herbig Ae/Be stars - Evidence for Disks and Envelopes

76 citations · 813 across the 32 of their papers we have counts for

collaborators

31 papers

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.SR2022★ 5 cited

Instability in the system of the distant post-AGB star LS III+52 24 (IRAS 22023+5249)

V. G. Klochkova, A. S. Miroshnichenko, V. E. Panchuk +2

The optical spectra of the B-supergiant LS III+52 24 (IRAS 22023+5249) obtained at the 6-meter telescope BTA with a resolution R60000 in 2010-2021 revealed signs of wind varia…

astro-ph.SR2021★ 20 cited

Outbursts and stellar properties of the classical Be star HD 6226

Noel D. Richardson, Olivier Thizy, Jon E. Bjorkman +58

The bright and understudied classical Be star HD 6226 has exhibited multiple outbursts in the last several years during which the star grew a viscous decretion disk. We analyze 659…

astro-ph.SR2020★ 18 cited

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…

astro-ph.EP2018★ 6 cited

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…

astro-ph.SR2018★ 47 cited

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…