Welcome to the Star Formation Group
We study the physics of star formation from 100AU to 100kpc scales, from individual protostars in our Galaxy to compact groups of galaxies. This breadth allows us to ground galaxy-scale star formation in an understanding of the microphysics, and place individual nearby regions in broader environmental context. We use observational techniques from X-ray to centimeter, with particular recent focus on infrared and (sub)millimeter, as well as radiative transfer and other numerical models.
News

HERACLES Database
ALMA Early Science