Anatoly Miroshnichenko

Professor

University of North Carolina at Greensboro

United States

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Professor Anatoly Miroshnichenko is a faculty member at the University of North Carolina Greensboro, USA. His research primarily focuses on the study of binary star systems, the B[e] phenomenon, and spectral characteristics of various astronomical objects. Recent publications include investigations into the spectral and photometric properties of stars like MWC 342 and HD 698, as well as orbital parameter determination using MCMC methods.

Articles (20)

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2025

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2025

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2025

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2025

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2025

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2025

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2025

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2024

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2023

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2023

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2022

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2022

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2022

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2021

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2020

Collaborators (1)

Frederick Walter

Professor

Stony Brook University

UNITED STATES

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Anatoly Miroshnichenko

Research Interests

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Articles (20)

The Unexplored Dusty Nova LMCN 2009-05a in the Large Magellanic Cloud

Determination of Orbital Parameters of Binary Star Systems Using the MCMC Method

Doppler Tomography of the Be Star HD 698

Комплексный анализ спектральных и фотометрических характеристик объекта с феноменом B[E] MWC 342 за 40-летний период наблюдений

Searching for New Objects with the B[e] Phenomenon

A Spectroscopic and Photometric Study of MWC 342 and Its B[e] Phenomenon over the Last 40 Years

Fundamental Parameters and Evolutionary Scenario of HD 327083

IRAS 17449+2320: A Possible Binary System with the B[e] Phenomenon and a Strong Magnetic Field

HR 4049: A Spectroscopic Analysis of a Post-AGB Object

AS 314: A Massive Dusty Hypergiant or a Low-Mass Post-Asymptotic Giant Branch Object?

Properties of Galactic B[e] Supergiants. X. Refined Orbit and Fundamental Parameters of the HD 327083 Binary System

Doppler Tomography of the Circumstellar Disk of the Be Star κ Draconis

A variety of binary targets for small telescopes

Searching for Phase-Locked Variations of the Emission-Line Profiles in Binary Be Stars

Recent Progress in Finding Binary Systems with the B[e] Phenomenon

Refining Orbits of Bright Binary Systems

Toward Understanding the B[e] Phenomenon. IX. Nature and Binarity of MWC645

Toward Understanding the B[e] Phenomenon. VIII. Nature and Variability of IRAS 07080+0605

First high-resolution optical spectra of the distant emission-line star VES 723 (IRAS 02110+6212)

Properties of Galactic B[e] Supergiants. V. 3 Pup–Constraining the Orbital Parameters and Modeling the Circumstellar Environments

Collaborators (1)

Frederick Walter

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