activity
20242026
collaborators

14 papers

astro-ph.EP2026

Asymmetric, variable H line profile in planetary mass object SR 12 c

Jun Hashimoto, Yuhiko Aoyama, Michihiro Takami +1

Young, forming planetary-mass objects often exhibit clear signatures of ongoing mass accretion and are thought to accrete material through processes analogous to those operating in…

astro-ph.GA2026

Cosmic ray heating of cold streams: Implications for the gas supply and growth of massive galaxies

Ellis R. Owen, Nicolas Ledos, Evangelia Ntormousi +3

Recent observations have demonstrated the presence of cosmic rays (CRs) in cosmic-web filaments. Cold streams supply gas inflows from these filaments into massive galaxies during t…

astro-ph.IM2026

Systematic Comparison between Constrained Transport and Mixed Divergence Cleaning Methods for Astrophysical Magnetohydrodynamic Simulations

Kengo Tomida, Kenji Eric Sadanari, Shinsuke Takasao +1

Magnetohydrodynamic (MHD) simulations are indispensable research infrastructure in astrophysics today. In order to satisfy the solenoidal constraint of the MHD equations on discret…

astro-ph.SR2026

Numerical Investigation of Efficient Electron Acceleration at an Unsteady Solar Flare Loop-Top

Yoshiaki Sato, Takafumi Kaneko, Noriyuki Narukage +1

Using magnetohydrodynamic (MHD) fields and guiding-center test-particle calculations, this study investigates how time-dependent loop-top dynamics modulate the adiabatic energizati…

astro-ph.GA2026

A Magnetized Black Hole Envelope Model for Little Red Dots

Shinsuke Takasao, Kohei Inayoshi

Recent observations have revealed a unique class of active galactic nuclei (AGNs), termed little red dots (LRDs). These objects are hypothesized to be powered by massive black hole…

astro-ph.GA2026

The hydrodynamical response of cold circumgalactic clouds to quasar radiation

Nicolas Ledos, Sebastiano Cantalupo, Titouan Lazeyras +8

Recent simulations increasingly resolve the small-scale structure of the circumgalactic medium (CGM), but the dynamical impact of ionising radiation on its cold K component…