X-factor (astrophysics)


The X-factor in astrophysics, often labeled XCO, is an empirically determined proportionality constant which converts carbon monoxide emission line brightness to molecular hydrogen mass.

Origin

The term X-factor was coined in a 1983 paper titled "Gamma-rays from atomic and molecular gas in the first galactic quadrant" and published in The Astrophysical Journal.

Calibration

Calibrating XCO requires an independent method of determining the amount of molecular hydrogen in a given astrophysical region. While direct emission from molecular hydrogen is difficult to observe, there are other ways of inferring molecular hydrogen mass, outlined below.