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...

Detaylı Bibliyografya
Asıl Yazarlar:	Takumi Ohmura, Mami Machida, Kenji Nakamura, Yuki Kudoh, Yuta Asahina, Ryoji Matsumoto
Materyal Türü:	Makale
Dil:	English
Baskı/Yayın Bilgisi:	MDPI AG 2019-01-01
Seri Bilgileri:	Galaxies
Konular:	astrophysical jets magnetohydrodynamics (MHD) numerical simulation
Online Erişim:	http://www.mdpi.com/2075-4434/7/1/14

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