activity
20242026
collaborators

6 papers

astro-ph.SR2026

Dynamical friction in stratified stellar envelopes

Damien Gagnier

Dynamical friction prescriptions used for common-envelope and planetary engulfment inspirals often assume a homogeneous medium and/or rectilinear perturber motion. A gravitating ob…

astro-ph.SR2026

Continuous mass ablation of planets engulfed in stellar envelopes

Mike Y. M. Lau, Robert Andrassy, Giovanni Leidi +4

Most stars host short-period planets that are expected to be engulfed during post-main-sequence expansion. The dissolution of engulfed planets has been proposed as a possible mecha…

astro-ph.SR2026

Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics

G. Leidi, A. Holas, K. Vitovsky +11

We present PHLEGETHON, a fully compressible, Eulerian magnetohydrodynamic (MHD) code designed for multidimensional simulations in stellar astrophysics. The code uses a time-explici…

astro-ph.SR2026

Local simulations of common-envelope dynamical inspiral. Impact of rotation, accretion, and stratification

D. Gagnier, G. Leidi, M. Vetter +2

Common envelope evolution (CEE) is a crucial phase in binary stellar evolution. Current global three-dimensional simulations lack the resolution to capture the small-scale dynamics…

astro-ph.SR2025

Magnetically driven outflows in 3D common-envelope evolution of massive stars

Marco Vetter, Friedrich K. Roepke, Fabian R. N. Schneider +7

Recent three-dimensional magnetohydrodynamical simulations of the common-envelope interaction revealed the self-consistent formation of bipolar magnetically driven outflows launche…

astro-ph.SR2024

Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral

Damien Gagnier, Ondrej Pejcha

Three-dimensional hydrodynamical simulations of common envelope evolution are often terminated soon after the initial dynamical plunge of the companion transitions into a long-last…