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...

書目詳細資料
Main Authors:	Takumi Ohmura, Mami Machida, Kenji Nakamura, Yuki Kudoh, Yuta Asahina, Ryoji Matsumoto
格式:	Article
語言:	English
出版:	MDPI AG 2019-01-01
叢編:	Galaxies
主題:	astrophysical jets magnetohydrodynamics (MHD) numerical simulation
在線閱讀:	http://www.mdpi.com/2075-4434/7/1/14

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