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...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Egile nagusia: Castro Piña, Juan Andrés (author)
Formatua: bachelorThesis
Argitaratua: 2025
Gaiak:
Sarrera elektronikoa:https://repositorio.yachaytech.edu.ec/handle/123456789/1030
Etiketak: Etiketa erantsi
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