A detailed view of filaments and sheets in the warm-hot intergalactic medium

DOI10.1051/0004-6361/201014040zbMath1260.85136arXiv1008.2311OpenAlexW3105977332WikidataQ68974573 ScholiaQ68974573MaRDI QIDQ4905527

Jan P. Mücket, J. S. Klar

Publication date: 19 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1008.2311

zbMATH Keywords

cosmologyhydrodynamicsmethods: numericalintergalactic medium

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Astrophysical cosmology (85A40)

Related Items (7)

On the Stability of Unconditionally Positive and Linear Invariants Preserving Time Integration Schemes ⋮ On Lyapunov stability of positive and conservative time integrators and application to second order modified Patankar–Runge–Kutta schemes ⋮ On order conditions for modified Patankar-Runge-Kutta schemes ⋮ Extension of modified Patankar-Runge-Kutta schemes to nonautonomous production-destruction systems based on Oliver's approach ⋮ Analytic growth rate of gravitational instability in self-gravitating planar polytropes ⋮ Unconditionally positive and conservative third order modified Patankar-Runge-Kutta discretizations of production-destruction systems ⋮ On the existence of three-stage third-order modified Patankar-Runge-Kutta schemes

This page was built for publication: A detailed view of filaments and sheets in the warm-hot intergalactic medium