The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation
arXiv:1901.05467 · doi:10.1093/mnras/stz1692
Abstract
We exploit EAGLE, a cosmological hydrodynamical simulation, to reproduce the selection of the observed sub-millimeter (submm) galaxy population by selecting the model galaxies at with mock submm fluxes mJy. There is a reasonable agreement between the galaxies within this sample and the properties of the observed submm population, such as their star formation rates (SFRs) at , redshift distribution and many integrated galaxy properties. We find that the bulk of the mJy model population is at , and that they are massive galaxies ( Msol) with high dust masses ( Msol), gas fractions (%) and SFRs ( Msol/yr). They have major and minor merger fractions similar to the general population, suggesting that mergers are not the primary driver of the model submm galaxies. Instead, the mJy model galaxies yield high SFRs primarily because they maintain a significant gas reservoir as a result of hosting an undermassive black hole. In addition, we find that not all highly star-forming EAGLE galaxies have submm fluxes mJy. Thus, we investigate the nature of highly star-forming Submm-Faint galaxies (i.e., Msol/yr but mJy). We find they are similar to the model submm galaxies; being gas rich and hosting undermassive black holes, however they are typically lower mass ( Msol) and are at higher redshifts (). These typically higher- galaxies show stronger evidence for having been triggered by major mergers, and critically, they are likely missed by current submm surveys due to their higher dust temperatures. This suggests a potentially even larger contribution to the SFR density at from dust-obscured systems than implied by current observations.
arXiv comment15 pages, 9 figures, submitted to MNRAS
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