2007/11/29 by Sara L. Ellison, David R. Patton, Luc Simard +1 · 4 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Elliptical galaxy #Extragalactic astronomy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Luminous infrared galaxy #Scientific Research and Discoveries #Sky #Star formation #Stellar mass #astro-ph
paper · pdf · doi:10.1086/527296
Accepted by ApJ Letters
arxiv created 2007/11/29 · openalex publication_date 2007/12/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We use a sample of 43,690 galaxies selected from the Sloan Digital Sky Survey Data Release 4 to study the systematic effects of specific star formation rate (SSFR) and galaxy size (as measured by the half-light radius, r h ) on the mass-metallicity relation. We find that galaxies with high SSFR or large r h for their stellar mass have systematically lower gas-phase metallicities (by up to 0.2 dex) than galaxies with low SSFR or small r h . We discuss possible origins for these dependencies, including galactic winds/outflows, abundance gradients, environment, and star formation rate efficiencies.