Fast Outflows in Hot Dust-Obscured Galaxies with Keck/NIRES

Abstract

We present rest-frame optical spectroscopic observations of 24 Hot Dust-Obscured Galaxies (Hot DOGs) at redshifts 1.7-4.6 with KECK/NIRES. Our targets are selected based on their extreme red colors to be the highest luminosity sources from the WISE infrared survey. In 20 sources with well-detected emission we fit the key [O III], H${\hat{I}}^2$, H$\hat{I}\pm$, [N II], and [S II] diagnostic lines to constrain physical conditions. Of the 17 targets with a clear detection of the [O III]$\hat{\mathrm{I}}»$5007A emission line, 15 display broad blueshifted and asymmetric line profiles, with widths ranging from 1000 to 8000 $\mathrm{km}{\mathrm{s}}^{-1}$ and blueshifts up to 3000 $\mathrm{km}{\mathrm{s}}^{-1}$. These kinematics provide strong evidence for the presence of massive ionized outflows of up to $8000{\mathrm{M}}_{\odot }\mathrm{y}{\mathrm{r}}^{-1}$, with a median of $150{\mathrm{M}}_{\odot }\mathrm{y}{\mathrm{r}}^{-1}$. As many as eight sources show optical emission line ratios consistent with vigorous star formation. Balmer line star-formation rates, uncorrected for reddening, range from 30--1300 ${\mathrm{M}}_{\odot }\mathrm{y}{\mathrm{r}}^{-1}$, with a median of $50{\mathrm{M}}_{\odot }\mathrm{y}{\mathrm{r}}^{-1}$. Estimates of the SFR from SED fitting of mid and far-infrared photometry suggest significantly higher values. We estimate the central black hole masses to be of order $10^{8-10}{\mathrm{M}}_{\odot }$, assuming the present-day ${\mathrm{M}}_{\mathrm{BH}}-\ddot{\mathrm{I}}{ƒ}_{\ast }$ relation. The bolometric luminosities and the estimated masses of the central black holes of these galaxies suggest that many of the AGN-dominated Hot DOGs are accreting at or above their Eddington limit. The combination of ongoing star formation, massive outflows, and high Eddington ratios suggest Hot DOGs are a transitional phase in galaxy evolution.

26 pages, 5 figures, accepted to ApJ