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We analyze the cool gas in and around 14 nearby galaxies (at $z$$<$0.1)mapped with the SDSS-IV MaNGA survey by measuring absorption lines produced bygas in spectra of background quasars/AGN at impact parameters of 0-25 effectiveradii from the galaxy center. Using HST/COS, we detect absorption at the galaxyredshift and measure or constrain column densities of neutral (H I, N I, O I,Ar I), low-ionization (Si II, S II, C II, N II Fe II), and high-ionization (SiIII, Fe III, N V, O VI) species for 11 galaxies. We derive the ionizationparameter and ionization-corrected metallicity using CLOUDY photo-ionizationmodels. The H I column density ranges from $\sim$$10^{13}$ to$\sim$$10^{20}\,{\rm cm^{-2}}$ and decreases with impact parameter for $r \geR_{e}$. Galaxies with higher stellar mass have weaker H I absorption. Comparingabsorption velocities with MaNGA radial velocity maps of ionized gas lineemissions in galactic disks, we find that the neutral gas seen in absorptionco-rotates with the disk out to $\sim$10 $R_{e}$. Sight lines with lowerelevation angles show lower metallicities, consistent with the metallicitygradient in the disk derived from MaNGA maps. Higher elevation angle sightlines show higher ionization, lower H I-column density, super-solarmetallicity, and velocities consistent with the direction of galactic outflow.Our data offer the first detailed comparisons of CGM properties (kinematics andmetallicity) with extrapolations of detailed galaxy maps from integral fieldspectroscopy; similar studies for larger samples are needed to more fullyunderstand how galaxies interact with their CGM.

The Baryonic Content of Galaxies Mapped by MaNGA and the Gas Around Them