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...

書誌詳細
主要な著者:	Takumi Ohmura, Mami Machida, Kenji Nakamura, Yuki Kudoh, Yuta Asahina, Ryoji Matsumoto
フォーマット:	論文
言語:	English
出版事項:	MDPI AG 2019-01-01
シリーズ:	Galaxies
主題:	astrophysical jets magnetohydrodynamics (MHD) numerical simulation
オンライン･アクセス:	http://www.mdpi.com/2075-4434/7/1/14

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