Slow Star Formation in the Milky Way: Theory Meets Observations

TL;DR

This paper explains the Milky Way's star formation rate by integrating metallicity-dependent gas mass conversion and virial parameter-based efficiency, resolving long-standing discrepancies between observations and theory.

Contribution

It introduces a combined model incorporating metallicity effects and virial parameter dependence to accurately predict the Milky Way's star formation rate and its radial variation.

Findings

The model matches observed star formation rates within a factor of two.

It explains the radial trend of star formation surface density.

Resolves a 50-year-old discrepancy between observed and theoretical rates.

Abstract

The observed star formation rate of the Milky Way can be explained by applying a metallicity-dependent factor to convert CO luminosity to molecular gas mass and a star formation efficiency per free-fall time that depends on the virial parameter of a molecular cloud. These procedures also predict the trend of star formation rate surface density with Galactocentric radius. The efficiency per free-fall time variation with virial parameter plays the major role in bringing theory into agreement with observations for the total star formation rate, while the metallicity dependence of the CO luminosity to mass conversion is most notable in the variation with Galactocentric radius. Application of these changes resolves a factor of over 100 discrepancy between observed and theoretical star formation rates that has been known for nearly 50 years.