No sign of strong molecular gas outflow in an infrared-bright
  dust-obscured galaxy with strong ionized-gas outflow
  We report the discovery of an infrared (IR)-bright dust-obscured galaxy (DOG)
that shows a strong ionized-gas outflow but no significant molecular gas
outflow. Based on detail analysis of their optical spectra, we found some
peculiar IR-bright DOGs that show strong ionized-gas outflow
([OIII]$\lambda$5007) from the central active galactic nucleus (AGN). For one
of these DOGs (WISE J102905.90+050132.4) at $z_{\rm spec} = 0.493$, we
performed follow-up observations using ALMA to investigate their CO molecular
gas properties. As a result, we successfully detected $^{12}$CO($J$=2-1) and
$^{12}$CO($J$=4-3) lines, and the continuum of this DOG. The intensity-weighted
velocity map of both lines shows a gradient, and the line profile of those CO
lines is well-fitted by a single narrow Gaussian, meaning that this DOG has no
sign of strong molecular gas outflow. The IR luminosity of this object is
$\log\,(L_{\rm IR}/L_{\odot})$ = 12.40 that is classified as ultraluminous IR
galaxy (ULIRG). We found that (i) the stellar mass and star-formation rate
relation and (ii) the CO luminosity and far-IR luminosity relation are
consistent with those of typical ULIRGs at similar redshifts. These results
indicate that the molecular gas properties of this DOG are normal despite that
its optical spectrum showing a powerful AGN outflow. We conclude that a
powerful ionized-gas outflow caused by the AGN does not necessarily affect the
cold interstellar medium in the host galaxy at least for this DOG.
