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Two-dimensional MHD model of gas flow dynamics near a young star with a jet and a protoplanetary disk
Published online by Cambridge University Press: 20 January 2023
Abstract
A numerical nonstationary two-dimensional MHD model of a protoplanetary disk near T Tauri star with a jet is developed. The model assumes consideration of pure gas ionization, optically thin cooling, anisotropic thermal conductivity and viscosity. The relaxation of gas-dynamic flows is analyzed. Based on the evolution of plasma flows, profiles of hydrogen spectral lines have been obtained.
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- © The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union