Distribution and kinematics of the circumnuclear molecular gas in the Seyfert 1 galaxy NGC 3227

We present new interferometric observations of the (CO)-C-12 (1-0), (CO)-C-12 (2-1), and HCN (1-0) molecular line emission in NGC 3227 obtained with the IRAM Plateau de Bure interferometer (PdBI). We achieved an unprecedented angular resolution in the 12CO (2-1) line of about 0."6 corresponding to only about 50 pc at a distance of 17.3 Mpc. The mapped (CO)-C-12 emission is concentrated in the inner 8" and accounts for 20% of the total 30 m (CO)-C-12 line flux. The (CO)-C-12 emission is resolved into an asymmetric nuclear ring with a diameter of about 3". The HCN line emission is mostly unresolved at our resolution of similar to 2."4 and contains all of the single-dish flux. We have decomposed the observed molecular gas motions into a circular and noncircular component revealing that about 80% of the gas in the circumnuclear region exhibits pure circular rotation. We find evidence for bar streaming onto the nuclear ring and a redshifted emission knot on the ring perimeter. In the central arcsecond the gas shows apparent counterrotation. This behavior can be best explained by a warping of the inner molecular gas disk rather than gas motion in a nuclear bar potential. We detected molecular gas at a distance from the nucleus of only similar to 13 pc with a velocity of about 75 km s(-1) with respect to the systemic velocity and find that within the central arcsecond the rotation curve is rising again. This is the first time that millimetric CO line emission has been detected interferometrically at such small distances to the nucleus of a Seyfert galaxy. These measurements indicate a lower limit on the enclosed mass of about 2 x 10(7) M. in the inner 25 pc.