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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Chi tiết về thư mục
Những tác giả chính:	Takumi Ohmura, Mami Machida, Kenji Nakamura, Yuki Kudoh, Yuta Asahina, Ryoji Matsumoto
Định dạng:	Bài viết
Ngôn ngữ:	English
Được phát hành:	MDPI AG 2019-01-01
Loạt:	Galaxies
Những chủ đề:	astrophysical jets magnetohydrodynamics (MHD) numerical simulation
Truy cập trực tuyến:	http://www.mdpi.com/2075-4434/7/1/14

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