activity
20172026
most citedSupernova Explosions in Accretion Disks in Active Galactic Nuclei: Three-Dimensional Models

21 citations · 48 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2026

Turbulence destroys thermal lobes around Mars-sized planetary embryos

R. O. Chametla, A. Moranchel-Basurto, F. J. Sánchez-Salcedo

The release of heat by a planetary embryo modifies the local density perturbations, forming thermal lobes in its vicinity, and thereby altering the torque exerted by the disk on th…

astro-ph.EP2025★ 2 cited

Dust back-reaction on gas around planets modifies the cold thermal torque

Raúl O. Chametla, Ondřej Chrenko, F. J. Sánchez-Salcedo +7

A nascent planet in a gas disk experiences radial migration due to the different torques which act on it. It has recently been shown that the torques produced by the gas and dust d…

astro-ph.SR2025

Multipolar magnetic configuration: a trace of post-mergers events in circumstellar disks around FS CMa Stars

A. Moranchel-Basurto, D. Kocakova, M. Cemeljic +3

Context: Observations suggest that magnetic fields of disk-bearing stars may have non-dipolar configurations. However, the influence of these configurations on magnetospheric accre…

astro-ph.SR2024★ 3 cited

2.5-MHD models of circumstellar discs around FS~CMa post-mergers : II. Stationary accretion stage

A. Moranchel-Basurto, D. Korčáková, R. O. Chametla

We study the star-disc interaction in the presence of the strong magnetic field () of a slowly rotating star. This situation describes a post-merger of the spectral…

astro-ph.SR2023★ 7 cited

2.5-MHD models of circumstellar discs around FS~CMa post-mergers : I. Non-stationary accretion stage

A. Moranchel-Basurto, D. Korčáková, R. O. Chametla

We investigate the dynamic evolution of gaseous region around FS~CMa post-mergers. Due to the slow rotation of a central B-type star, the dynamics is driven mainly by the magnetic…

astro-ph.HE2020★ 21 cited

Supernova Explosions in Accretion Disks in Active Galactic Nuclei: Three-Dimensional Models

A. Moranchel-Basurto, F. J. Sánchez-salcedo, Raúl O. Chametla +1

Supernova (SN) explosions can potentially affect the structure and evolution of circumnuclear disks in active galactic nuclei (AGN). Some previous studies have suggested that a rel…

astro-ph.HE2017★ 15 cited

A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case

P. F. Velázquez, E. M. Schneiter, E. M. Reynoso +6

Three dimensional magnetohydrodynamical simulations were carried out in order to perform a new polarization study of the radio emission of the supernova remnant SN 1006. These simu…