Why is the Milky Way X-factor Constant?
Desika Narayanan (Haverford College), Philip Hopkins (Caltech)

TL;DR
This study explains the near-constant CO-H2 conversion factor in the Milky Way by showing that stellar feedback regulates molecular cloud properties, leading to similar physical conditions across clouds.
Contribution
The paper demonstrates through high-resolution simulations that stellar feedback causes molecular clouds to have uniform properties, explaining the constant X-factor in the Milky Way.
Findings
Radiative feedback regulates cloud properties.
Cloud surface densities are similar due to feedback.
Feedback-free clouds have higher surface densities and X-factors.
Abstract
The CO-H2 conversion factor (Xco; otherwise known as the X-factor) is observed to be remarkably constant in the Milky Way and in the Local Group (aside from the SMC). To date, our understanding of why Xco should be so constant remains poor. Using a combination of extremely high resolution (~ 1 pc) galaxy evolution simulations and molecular line radiative transfer calculations, we suggest that Xco displays a narrow range of values in the Galaxy due to the fact that molecular clouds share very similar physical properties. In our models, this is itself a consequence of stellar feedback competing against gravitational collapse. GMCs whose lifetimes are regulated by radiative feedback show a narrow range of surface densities, temperatures and velocity dispersions with values comparable to those seen in the Milky Way. As a result, the X-factors from these clouds show reasonable correspondence…
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