activity
19982025
most citedThree-dimensional Simulations of Disk Accretion to an Inclined Dipole: II. Hot Spots and Variability

304 citations · 2.9k across the 39 of their papers we have counts for

collaborators

40 papers

astro-ph.EP2025★ 2 cited

3D MHD simulations of planet migration in cavities and inner discs of magnetized stars

M. M. Romanova, A. V. Koldoba, G. V. Ustyugova +2

We investigate the Type I migration of planets in low-density cavities and inner discs of strongly magnetized young stars using global three-dimensional (3D) magnetohydrodynamic (M…

astro-ph.EP2024

Eccentricity and Inclination of Massive Planets Inside Low-density Cavities: Results of 3D Simulations

M. M. Romanova, A. V. Koldoba, G. V. Ustyugova +2

We study the evolution of eccentricity and inclination of massive planets in low-density cavities of protoplanetary discs using three-dimensional (3D) simulations. When the planet'…

astro-ph.EP2023★ 9 cited

Eccentricity Growth of Massive Planets inside Cavities of Protoplanetary Discs

Marina M. Romanova, Alexander V. Koldoba, Galina V. Ustyugova +2

We carry out hydrodynamical simulations to study the eccentricity growth of a 1-30 Jupiter mass planet located inside the fixed cavity of a protoplanetary disc. The planet exchange…

astro-ph.SR2020★ 57 cited

3D MHD Simulations of Accretion onto Stars with Tilted Magnetic and Rotational Axes

M. M. Romanova, A. V. Koldoba, G. V. Ustyugova +3

We present results of global three-dimensional (3D) magnetohydrodynamic (MHD) simulations of accretion onto magnetized stars where both the magnetic and rotational axes of the star…

astro-ph.HE2019★ 26 cited

Modelling the interaction between relativistic and non-relativistic winds in binary pulsar systems: strong magnetization of the pulsar wind

Sergey V. Bogovalov, Dmitry Khangulyan, Alexander V. Koldoba +2

We present a numerical study of the properties of the flow produced by the collision of a magnetized anisotropic pulsar wind with the circumbinary environment. We focus on studying…

astro-ph.EP2018★ 33 cited

3D Simulations of Planet Trapping at Disc-Cavity Boundaries

M. M. Romanova, P. S. Lii, A. V. Koldoba +4

Inward migration of low-mass planets and embryos of giant planets can be stopped at the disc-cavity boundaries due to co-orbital corotation torque. We performed the first global th…