Simulations of common-envelope evolution in binary stellar systems: physical models and numerical techniques
FK Röpke, O De Marco - Living Reviews in Computational Astrophysics, 2023 - Springer
When the primary star in a close binary system evolves into a giant and engulfs its
companion, its core and the companion temporarily orbit each other inside a common …
companion, its core and the companion temporarily orbit each other inside a common …
Gamma-ray binaries and related systems
G Dubus - The Astronomy and Astrophysics Review, 2013 - Springer
After initial claims and a long hiatus, it is now established that several binary stars emit high-
(0.1–100 GeV) and very high-energy (> 100 GeV) gamma rays. A new class has emerged …
(0.1–100 GeV) and very high-energy (> 100 GeV) gamma rays. A new class has emerged …
Enzo: An adaptive mesh refinement code for astrophysics
This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
MPI-AMRVAC 3.0: Updates to an open-source simulation framework
Context. Computational astrophysics nowadays routinely combines grid-adaptive
capabilities with modern shock-capturing, high resolution spatio-temporal integration …
capabilities with modern shock-capturing, high resolution spatio-temporal integration …
The Athena++ adaptive mesh refinement framework: design and magnetohydrodynamic solvers
JM Stone, K Tomida, CJ White… - The Astrophysical …, 2020 - iopscience.iop.org
The design and implementation of a new framework for adaptive mesh refinement
calculations are described. It is intended primarily for applications in astrophysical fluid …
calculations are described. It is intended primarily for applications in astrophysical fluid …
Essentially non-oscillatory and weighted essentially non-oscillatory schemes
CW Shu - Acta Numerica, 2020 - cambridge.org
Essentially non-oscillatory (ENO) and weighted ENO (WENO) schemes were designed for
solving hyperbolic and convection–diffusion equations with possibly discontinuous solutions …
solving hyperbolic and convection–diffusion equations with possibly discontinuous solutions …
The black hole accretion code
We present the black hole accretion code (BHAC), a new multidimensional general-
relativistic magnetohydrodynamics module for the MPI-AMRVAC framework. BHAC has …
relativistic magnetohydrodynamics module for the MPI-AMRVAC framework. BHAC has …
MPI-AMRVAC for solar and astrophysics
O Porth, C ** atmospheres of hot gas planets in the solar neighborhood
M Salz, S Czesla, PC Schneider, J Schmitt - Astronomy & Astrophysics, 2016 - aanda.org
Absorption of high-energy radiation in planetary thermospheres is generally believed to lead
to the formation of planetary winds. The resulting mass-loss rates can affect the evolution …
to the formation of planetary winds. The resulting mass-loss rates can affect the evolution …