Galaxy metallicities depend primarily on stellar mass and molecular gas mass
1 Cavendish Laboratory, University of
Cambridge, 19 J.J. Thomson
Avenue, Cambridge CB3
2 Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
3 ETH Zurich, Institute for Astronomy, Wolfgang-Pauli-Strasse 27, 8093 Zurich, Switzerland
4 Kavli Institute for Astronomy and Astrophysics, Peking University, 100871 Beijing, PR China
5 SKA Organisation, Lower Withington, Macclesfield, Cheshire, SK11 9DL, UK
Accepted: 10 June 2016
Aims. We present an analysis of the behaviour of galaxies in a four-dimensional parameter space defined by stellar mass, metallicity, star formation rate, and molecular gas mass. We analyse a combined sample of 227 galaxies that draws from a number of surveys across the redshift range 0 < z < 2 (>90% of the sample at z ~ 0) and covers >3 decades in stellar mass.
Methods. Using principal component analysis, we demonstrate that galaxies in our sample lie on a 2D plane within this 4D parameter space, which is indicative of galaxies that exist in an equilibrium between gas inflow and outflow. Furthermore, we find that the metallicity of galaxies depends only on stellar mass and molecular gas mass. In other words, gas-phase metallicity has a negligible dependence on star formation rate once the correlated effect of molecular gas content is accounted for.
Results. The well-known fundamental metallicity relation which describes a close and tight relationship between metallicity and SFR (at fixed stellar mass) is therefore entirely a by-product of the underlying physical relationship with molecular gas mass (through the Schmidt-Kennicutt relation).
Key words: galaxies: ISM / galaxies: statistics / galaxies: evolution / galaxies: abundances
© ESO, 2016