Galaxy and mass assembly (GAMA): The connection between metals, specific SFR and Hi gas in galaxies: The Z-SSFR relation

Lara-Lopez, M AHopkins, Andrew M.Lopez-Sanchez, A RBrough, SarahColless, MatthewBland-Hawthorn, JossDriver, Simon PFoster, CLiske, JochenLoveday, JRobotham, A. S. G.Sharp, Robert2015-12-130035-8711http://hdl.handle.net/1885/74619We study the interplay between gas phase metallicity (Z), specific star formation rate (SSFR) and neutral hydrogen gas (HI) for galaxies of different stellar masses. Our study uses spectroscopic data from Galaxy and Mass Assembly and Sloan Digital Sky SurAuthor/s retain copyrightKeywords: Galaxies: Abundances; Galaxies: Statistics.; Galaxies:Fundamental parameters; Galaxies:Star formationGalaxy and mass assembly (GAMA): The connection between metals, specific SFR and Hi gas in galaxies: The Z-SSFR relation201310.1093/mnrasl/slt0542016-02-24