Cold and warm molecular gas in the outflow of 4C12.50
K. M. Dasyra, F. Combes

TL;DR
This study uses radio observations to analyze the cold molecular gas in the outflow of galaxy 4C12.50, revealing its properties and estimating its mass, thereby shedding light on galaxy feedback processes.
Contribution
First detection of cold molecular gas in the outflow of 4C12.50 using CO lines, providing new constraints on its temperature and mass.
Findings
Cold H2 mass in outflow is at least 4.2×10^3 solar masses.
Outflowing cold gas constitutes about 37% of the warm gas component.
Estimated cold gas excitation temperature is >=65K.
Abstract
We present deep observations of the 12CO(1-0) and (3-2) lines in the ultra-luminous infrared and radio galaxy 4C12.50, carried out with the 30m telescope of the Institut de Radioastronomie Millimetrique. Our observations reveal the cold molecular gas component of a warm molecular gas outflow that was previously known from Spitzer Space Telescope data. The 12CO(3-2) profile indicates the presence of absorption at -950 km/s from systemic velocity with a central optical depth of 0.22. Its profile is similar to that of the HI absorption that was seen in radio data of this source. A potential detection of the (0-1) absorption enabled us to place an upper limit of 0.03 on its central optical depth, and to constrain the excitation temperature of the outflowing CO gas to >=65K assuming that the gas is thermalized. If the molecular clouds fully obscure the background millimeter continuum that is…
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