The Observed Relation between Stellar Mass, Dust Extinction and Star Formation Rate in Local Galaxies

TL;DR

This study analyzes how dust extinction correlates with star formation rate and stellar mass in local galaxies, revealing a mass-dependent switch from anti-correlation to positive correlation around 10^10 solar masses.

Contribution

It uncovers a mass-dependent relation between dust extinction and SFR, providing new insights into galaxy evolution and chemical processes.

Findings

Anti-correlation between dust extinction and SFR at stellar masses <10^10 M_solar.

Positive correlation between dust extinction and SFR at stellar masses >10^10 M_solar.

Extension of the SFR-dust extinction relation to quiescent galaxies.

Abstract

In this study we investigate the relation between stellar mass, dust extinction and star formation rate (SFR) using ~150,000 star-forming galaxies from the SDSS DR7. We show that the relation between dust extinction and SFR changes with stellar mass. For galaxies at the same stellar mass dust extinction is anti-correlated with the SFR at stellar masses <10^10 M_solar. There is a sharp transition in the relation at a stellar mass of 10^10 M_solar. At larger stellar masses dust extinction is positively correlated with the SFR for galaxies at the same stellar mass. The observed relation between stellar mass, dust extinction and SFR presented in this study helps to confirm similar trends observed in the relation between stellar mass, metallicity and SFR. The relation reported in this study provides important new constraints on the physical processes governing the chemical evolution of galaxies. The correlation between SFR and dust extinction for galaxies with stellar masses >10^10 M_solar is shown to extend to the population of quiescent galaxies suggesting that the physical processes responsible for the observed relation between stellar mass, dust extinction and SFR may be related to the processes leading to the shut down of star formation in galaxies.