Keywords
ISM: turbulences
ISM: SNR and superbubbles
Galaxies: kinematics and dynamics
ISM: SNR and superbubbles
Galaxies: kinematics and dynamics
How to Cite
Galaxy evolution-Star formation connection: from pc to kpc scales. (2014). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 44, 84-84. https://astronomia.unam.mx/journals/rmxac/article/view/2014rmxac..44...84m
Abstract
Energization of the interstellar medium by supernova explosions covers a crucial role in a number of astrophysical situations. Supernova explosions are important for the gas evolution on small scales, because they drive turbulence and are able to provide a self-regulation mechanism for star formation. Besides, their blast waves may also form molecular clouds by sweeping gas into a turbulent flow.
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