activity
20062025
most citedAccretion dynamics in the classical T Tauri star V2129 Oph

89 citations · 134 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025

Unstable accretion in TW Hya: 3D simulations and comparisons with observations

M. M. Romanova, C. C. Espaillat, J. Wendeborn +3

We investigate the origin of photometric variability in the classical T Tauri star TW Hya by comparing light curves obtained by TESS and ground-based telescopes with light curves c…

astro-ph.SR2023★ 5 cited

Density streams in the disc winds of Classical T Tauri stars

P. P. Petrov, K. N. Grankin, E. V. Babina +5

Spectral and photometric variability of the Classical T Tauri stars RY Tau and SU Aur from 2013 to 2022 is analyzed. We find that in SU Aur the H-alpha line's flux at radial veloci…

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…

astro-ph.SR2012★ 89 cited

Accretion dynamics in the classical T Tauri star V2129 Oph

S. H. P. Alencar, J. Bouvier, F. M. Walter +9

We analyze the photometric and spectroscopic variability of the classical T Tauri star V2129 Oph over several rotational cycles to test the dynamical predictions of magnetospheric…

astro-ph2006★ 7 cited

Torsional Magnetic Oscillations in Type I X-Ray Bursts

Richard V. E. Lovelace, Akshay K. Kulkarni, Marina M. Romanova

Thermonuclear burning on the surface of a neutron star causes the expansion of a thin outer layer of the star, . The layer rotates slower than the star due to angular moment…