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...
| প্রধান লেখক: | , , , , , |
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| বিন্যাস: | প্রবন্ধ |
| ভাষা: | English |
| প্রকাশিত: |
MDPI AG
2019-01-01
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| মালা: | Galaxies |
| বিষয়গুলি: | |
| অনলাইন ব্যবহার করুন: | http://www.mdpi.com/2075-4434/7/1/14 |