Magnetohydrodynamics of dense gas in multi-phase galactic winds
Numerical simulations of wind–cloud systems are essential for understanding the survival of dense gas clouds embedded in hot, diffuse galactic winds. While single-cloud studies have shown that magnetic fields, particularly those transverse to the wind, can shield clouds from ablation through magneti...
Gorde:
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| Formatua: | bachelorThesis |
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2025
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| Sarrera elektronikoa: | https://repositorio.yachaytech.edu.ec/handle/123456789/1030 |
| Etiketak: |
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