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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Bibliografiska uppgifter
Huvudupphovsmän: Takumi Ohmura, Mami Machida, Kenji Nakamura, Yuki Kudoh, Yuta Asahina, Ryoji Matsumoto
Materialtyp: Artikel
Språk:English
Publicerad: MDPI AG 2019-01-01
Serie:Galaxies
Ämnen:
astrophysical jets
magnetohydrodynamics (MHD)
numerical simulation
Länkar:http://www.mdpi.com/2075-4434/7/1/14

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