A pebble accretion model for the formation of the terrestrial planets in the Solar System. [PDF]
Johansen A +6 more
europepmc +1 more source
Simulations of Relativistic Force‐free Magnetohydrodynamic Turbulence
We present numerical studies of 3-dimensional magnetohydrodynamic (MHD) turbulence in a strongly magnetized medium in the extremely relativistic limit, in which the inertia of the charge carriers can be neglected. We have focused on strong Alfvenic turbulence in the limit. We have found the following results.
openaire +2 more sources
The Life and Times of Star-forming Cores: An Analysis of Dense Gas in the STARFORGE Simulations
Dense gas in molecular clouds is an important signature of ongoing and future star formation. We identify and track dense cores in the starforge simulations, following the core evolution from birth through dispersal by stellar feedback for typical Milky ...
Stella S. R. Offner +2 more
doaj +1 more source
The Interaction of a Supernova Remnant with Background Interstellar Turbulence
Supernova explosions are among the most energetic events in the Universe. After the explosion, the material ejected by the supernova expands throughout the interstellar medium (ISM), forming what is called a supernova remnant (SNR). The shocks associated
Giuseppe Prete +4 more
doaj +1 more source
Simulations of cosmic ray propagation. [PDF]
Hanasz M, Strong AW, Girichidis P.
europepmc +1 more source
Cosmic-Ray Acceleration of Galactic Outflows in Multiphase Gas
We investigate the dynamical interaction between cosmic rays (CRs) and the multiphase interstellar medium (ISM) using numerical magnetohydrodynamic (MHD) simulations with a two-moment CR solver and TIGRESS simulations of star-forming galactic disks.
Lucia Armillotta +3 more
doaj +1 more source
The Impact of Enhanced Extreme-ultraviolet Flux on the Upper Atmosphere of Earth-like Exoplanets
Identifying Earth-like planets outside our solar system is a leading research goal in astronomy, but determining if candidate planets have atmospheres, and more importantly if they can retain atmospheres, is still out of reach.
Lukas Hanson +3 more
doaj +1 more source
Odd Radio Circles Modeled by Shock-bubble Interactions
The physical nature and origins of the newly discovered class of Odd Radio Circles (ORCs) remain unclear. We investigate a model whereby ORCs are synchrotron-emitting vortex rings formed by the Richtmyer–Meshkov instability (RMI) when a shock interacts ...
Yiting Wang, Sebastian Heinz
doaj +1 more source
Effects of Dynamo-generated Large-scale Magnetic Fields on the Surface Gravity (f) Mode
By modeling the upper layers of the Sun in terms of a two-layer setup where a free surface exists within the computational domain, we numerically study the interaction between the surface gravity, or the fundamental ( f ) mode, and the magnetic fields ...
Rajesh Mondal, Nishant K. Singh
doaj +1 more source
Resistive Magnetohydrodynamics Simulation of Fusion Plasmas [PDF]
Tang, X.Z. +5 more
openaire +2 more sources

