arXiv:1401.4761 Abstract | arXiv Analytics

arXiv:1401.4761 [astro-ph.SR]Abstract References Reviews Resources

Simulations of Accretion onto Magnetized Stars: Results of 3D MHD Simulations and 3D Radiative Transfer

Published 2014-01-20Version 1

We discuss the results of modelling of young magnetized stars, where matter flow is calculated using the three-dimensional (3D) magneto-hydrodynamic (MHD) "Cubed Sphere" code, and the spectra are calculated using the 3D Monte Carlo radiative transfer code "TORUS". Two examples of modelling are shown: (1) accretion onto stars in stable and unstable regimes, and (2) accretion to a young star V2129 Oph, modelled with realistic parameters.

Comments: 6 pages, 5 figures, to appear in the proceedings of ASTRONUM-2013 meeting: "8th International Conference on Numerical Modeling of Space Plasma Flows", Biarritz, France, July 1-5, 2013

Categories: astro-ph.SR

Keywords: 3d mhd simulations, 3d radiative transfer, magnetized stars, monte carlo radiative transfer code, 3d monte carlo radiative transfer

Tags: conference paper

Related articles: Most relevant | Search more

arXiv:2212.11016 [astro-ph.SR] (Published 2022-12-21)

Progress towards a 3D Monte Carlo radiative transfer code for outflow wind modelling

Jakub Fišák, Jiří Kubát, Brankica Kubátová, Markus Kromer, Jiří Krtička

arXiv:2109.02971 [astro-ph.SR] (Published 2021-09-07)

Acoustic wave properties in footpoints of coronal loops in 3D MHD simulations

Julia M. Riedl, Tom Van Doorsselaere, Fabio Reale, Marcel Goossens, Antonino Petralia, Paolo Pagano

arXiv:1605.04979 [astro-ph.SR] (Published 2016-05-16)

Accretion, Outflows, and Winds of Magnetized Stars