A view of shocks and time-scales in galactic wind-cloud models

Wind-cloud models have been essential in understanding the small-scale processes occurring in galactic winds. Shocks are generated during such interactions. Some shock waves emerge in the ambient medium and some are internal to the cloud. The internal shocks can compress the gas on time-scales of th...

• Huvudupphovsman: Pinargote Morrillo, Bryan Joel (author)
• Materialtyp: bachelorThesis
• Språk: eng
• Publicerad: 2024
• Ämnen: Medio interestelar; Hidrodinámica; Simulaciones; Interstellar medium; Hydrodynamics; Simulations
• Länkar: http://repositorio.yachaytech.edu.ec/handle/123456789/860