Properties of cold molecular gas in four type-1 active galaxies hosting
  outflows
  Feedback from active galactic nuclei (AGN) has proven to be a critical
ingredient in the current picture of galaxy assembly and growth. However,
observational constraints on AGN-driven outflows face technical challenges and
as a result, the cold molecular gas outflow properties of type-1 AGN are not
well known. We present new IRAM NOrthern Extended Milimeter Array (NOEMA)
observations of CO (1-0) in F07599+6508, Z11598$-$0112, F13342+3932, and
PG1440+356, all nearby type-1 AGN and ultraluminous infrared galaxies (ULIRGs).
We achieve spatial resolution of 1-3 arcsec corresponding to physical scales of
2--8~kpc and spectral resolution of 15-60 km s$^{-1}$ which enables updated CO
(1-0) redshifts and a detailed morphological view of the cold molecular gas in
these sources. The CO (1-0) luminosities, $L_{CO}^{\prime}$, are in the range
2-12$\times 10^9$ K km s$^{-1}$ pc$^{2}$ and inferred molecular gas masses,
$M$(H$_2$), are in the range 2-9$\times 10^9$ M$_{\odot}$. The velocity fields
and gas distributions do not unambiguously identify any of these sources as
having outflows. However, Z11598$-$0112 has signs of infalling material and
after the subtraction of a rotating disk model PG 1440+356 shows complex
kinematics in the residuals that may indicate an outflow or warped disk.
