Electron–Ion Temperature Ratio in Astrophysical Shocks
Collisionless shock waves in supernova remnants and the solar wind heat electrons less effectively than they heat ions, as is predicted by kinetic simulations. However, the values of T _e / T _p inferred from the H α profiles of supernova remnant shocks behave differently as a function of Mach numbe...
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| Главные авторы: | , , , , , , , , , , , |
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| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
IOP Publishing
2023-01-01
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| Серии: | The Astrophysical Journal |
| Предметы: | |
| Online-ссылка: | https://doi.org/10.3847/1538-4357/acc528 |
| Метки: |
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