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...
| Päätekijät: | , , , , , |
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| Aineistotyyppi: | Artikkeli |
| Kieli: | English |
| Julkaistu: |
MDPI AG
2019-01-01
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| Sarja: | Galaxies |
| Aiheet: | |
| Linkit: | http://www.mdpi.com/2075-4434/7/1/14 |