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19942025
most citedThree-dimensional Simulations of Disk Accretion to an Inclined Dipole: II. Hot Spots and Variability

304 citations · 6.2k across the 108 of their papers we have counts for

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Showing 2013Show all

12 papers · 1 filter

astro-ph.SR2013★ 55 cited

Rossby Wave Instability in Astrophysical Discs

R. V. E. Lovelace, M. M. Romanova

A brief review is given of the Rossby wave instability (RWI) in astrophysical discs. In non-self-gravitating discs, around for example a newly forming stars, the instability can be…

astro-ph.SR2013★ 13 cited

MHD Simulations of Magnetospheric Accretion, Ejection and Plasma-field Interaction

M. M. Romanova, R. V. E. Lovelace, M. Bachetti +5

We review recent axisymmetric and three-dimensional (3D) magnetohydrodynamic (MHD) numerical simulations of magnetospheric accretion, plasma-field interaction and outflows from the…

astro-ph.EP2013★ 1 cited

The effect of an ordered azimuthal magnetic field on a migrating planet in a non-turbulent disc

M. L. Comins, M. M. Romanova, A. V. Koldoba +2

In this work, we consider the physics of the interaction between a planet and a magnetized gaseous protoplanetary disc. We investigate the migration of a planet in a disc that is t…

astro-ph.SR2013

Magnetospheric Accretions and the Inner Winds of Classical T Tauri Stars

Ryuichi Kurosawa, M. M. Romanova

Recent spectropolarimetric observations suggest that young low-mass stars such as classical T Tauri stars (CTTSs) possess relatively strong (~kG) magnetic field. This supports a sc…

astro-ph.SR2013★ 1 cited

Oscillations of the Boundary Layer and High-frequency QPOs

A. A. Blinova, M. Bachetti, M. M. Romanova

We observed persistent high-frequency oscillations of the boundary layer near an accreting, weakly-magnetized star in global 3D MHD simulations. The tilted dipole magnetic field is…

astro-ph.SR2013★ 1 cited

Boundary Between Stable and Unstable Regimes of Accretion

A. A. Blinova, R. V. E. Lovelace, M. M. Romanova

We investigated the boundary between stable and unstable regimes of accretion and its dependence on different parameters. Simulations were performed using a "cubed sphere" code wit…