activity
20242026
collaborators

9 papers

astro-ph.HE2026

Global simulations of accretion flows onto perturbers embedded in magnetized disks -I. MRI and jet formation in ideal MHD

Raúl O. Chametla, F. J. Sánchez-Salcedo, Martin E. Pessah +1

We present the highest resolution global MHD simulations to date of gas flow around a low mass a perturber with mass ratio , embedded in an accretion disk ar…

astro-ph.SR2026

Intermediate-Mass Mergers: A New Scenario for Several FS CMa Stars

Daniela Korcakova, Nela Dvorakova, Iris Bermejo Lozano +6

We summarise the properties and nature of a peculiar group of B-type stars called FS CMa stars. These stars show the B[e] phenomenon, i.e., their spectra exhibit both forbidden emi…

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

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.EP2025

Resurgence of CO in a warm bubble around accreting protoplanets and its observability

O. Chrenko, S. Casassus, R. O. Chametla

The cold outer regions of protoplanetary disks are expected to contain a midplane-centered layer where gas-phase CO molecules freeze out and their overall abundance is low. The lay…