Two-Temperature Magnetohydrodynamics Simulations of Propagation of Semi-Relativistic Jets

Two-Temperature Magnetohydrodynamics Simulations of Propagation of Semi-Relativistic Jets

In astrophysical jets observed in active galactic nuclei and in microquasars, the energy exchange rate by Coulomb collision is insufficient for thermal equilibrium between ions and electrons. Therefore, it is necessary to consider the difference between the ion temperature and the electron temperatu...

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Bibliografische gegevens
Hoofdauteurs:	Takumi Ohmura, Mami Machida, Kenji Nakamura, Yuki Kudoh, Yuta Asahina, Ryoji Matsumoto
Formaat:	Artikel
Taal:	English
Gepubliceerd in:	MDPI AG 2019-01-01
Reeks:	Galaxies
Onderwerpen:	astrophysical jets magnetohydrodynamics (MHD) numerical simulation
Online toegang:	http://www.mdpi.com/2075-4434/7/1/14

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