The interstellar medium  

At the end of the course, the student has a detailed knowledge of the observational and physical properties of the interstellar medium (ISM). In particular, the student acquires knowledge of the main constituents of the ISM (ionized, atomic, and molecular gas; dust; magnetic fields; cosmic rays; EM radiation), the different environments in which these are encountered (the 2- and 3-phase models of the ISM) and the physical processes that govern them. In addition, the student will acquire some knowledge about the central role played by the ISM in the evolution of galaxies and AGN across the cosmic time.
no data
English
The interstellar medium
English

Funded by the European Union. Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or HaDEA. Neither the European Union nor the granting authority can be held responsible for them. The statements made herein do not necessarily have the consent or agreement of the ASTRAIOS Consortium. These represent the opinion and findings of the author(s).