The Bright and Dark Sides of High-redshift Starburst Galaxies from Herschel and Subaru Observations
Daddi, E.; Rodighiero, G.; Sanders, D. B.; Kartaltepe, J. S.; Silverman, J. D.; Franceschini, A.; Valentino, F.; Mainieri, V.; Calabrò, A.; Renzini, A.; Maier, C.; Jin, S.; Rodríguez-Muñoz, L.; Mancini, C.; Puglisi, A.; Kashino, D.; Man, A.; Darvish, B.
Italy, Germany, France, Japan, Switzerland, Denmark, China, United States, Austria
Abstract
We present rest-frame optical spectra from the FMOS-COSMOS survey of 12 z ∼ 1.6 Herschel starburst galaxies, with star formation rate (SFR) elevated by ×8, on average, above the star-forming main sequence (MS). Comparing the Hα to IR luminosity ratio and the Balmer decrement, we find that the optically thin regions of the sources contain on average only ∼10% of the total SFR, whereas ∼90% come from an extremely obscured component that is revealed only by far-IR observations and is optically thick even in Hα. We measure the [N II]6583/Hα ratio, suggesting that the less obscured regions have a metal content similar to that of the MS population at the same stellar masses and redshifts. However, our objects appear to be metal-rich outliers from the metallicity-SFR anticorrelation observed at fixed stellar mass for the MS population. The [S II]6732/[S II]6717 ratio from the average spectrum indicates an electron density n e ∼ 1100 cm-3 , larger than what was estimated for MS galaxies but only at the 1.5σ level. Our results provide supporting evidence that high-z MS outliers are analogous of local ULIRGs and are consistent with a major-merger origin for the starburst event.