Star formation, metallicity and dust properties derived from the StromloAPM galaxy survey spectra

Abstract

ABSTRA C T We have derived star formation rates (SFRs), gas-phase oxygen abundances and effective dust absorption optical depths for a sample of galaxies drawn from the Stromlo‐ APM redshift survey using the new model of Charlot & Longhetti (CLO1), which provides a physically consistent description of the effects of stars, gas and dust on the integrated spectra of galaxies. Our sample consists of 705 galaxies with measurements of the fluxes and equivalent widths of Ha ,[ OII] and one or both of [N II] and [S II]. For a subset of the galaxies, 60- and 100-mm IRAS fluxes are available. We compare the star formation rates derived using the model with those derived using standard estimators based on the Ha, the [O II] and the far-infrared luminosities of the galaxies. The CL01 SFR estimates agree well with those derived from the IRAS fluxes, but are typically a factor of ,3 higher than those derived from the Ha or the [O II] fluxes, even after the usual mean attenuation correction of AHaa 1 mag is applied to the data. We show that the reason for this discrepancy is that the standard Ha estimator neglects the absorption of ionizing photons by dust in H II regions and the contamination of Ha emission by stellar absorption. We also use our sample to study variations in star formation and metallicity as a function of galaxy absolute bJ magnitude. For this sample, the star formation rate per unit bJ luminosity is independent of magnitude. The gas-phase oxygen abundance does increase with bJ luminosity, although the scatter in metallicity at fixed magnitude is large.