Connecting Galactic and extragalactic outflows: From the Cygnus-X cluster to active galaxies

Molecular outflows are often detected originating from both protostellar and extragalactic sources. Studies of low-mass, isolated high-mass, sources reveal scaling relations connecting the force carried by an outflow properties source that drives it. The aim this work is to examine effects clustered star formation on their explore possibility varying greatly scale energetics consistent with being launched same physical processes. High-angular resolution CO J = 3-2 observations were used ten high-mass protostars in Cygnus-X molecular cloud, obtained at SMA as part PILS-Cygnus survey. From these data, was measured. In addition, extended sample outflow-force measurements assembled existing literature allow for a direct comparison two types outflows. all survey, forces found close agreement literature. reveals, 95\% confidence, Class 0 follow force--bolometric luminosity correlation. between similar envelope mass bolometric suggests has no significant effect We find strong indication having launch mechanism. existence such mechanism would enable development single universal model, although more required order verify connection.