Speaker
Simon Glover
(Universität Heidelberg)
Description
Numerical simulations of star formation and stellar feedback have now advanced to the point where they routinely include relatively sophisticated treatments of the microphysics of the ISM. However, much of the predictive power of these simulations can only be harnessed if we can convert their results into synthetic observables that can be compared with observations of the real ISM. In this talk, I will discuss our ongoing efforts to produce and analyze synthetic observations of the ISM on a variety of scales and will give some examples of what we can learn from these studies.
Author
Simon Glover
(Universität Heidelberg)