High resolution near-infrared spectro-imaging of NGC 7027

We present near-infrared spectro-imaging of the young planetary nebula NGC 7027 between 2.10 and 2.20 mum with high spatial (0.5) and high spectral (8.7 km s(-1)) resolution. The observations, made using BEAR at the CFHT, reveal the detailed morphology and kinematics of the ionized nebula (in the Brgamma line and 16 other atomic lines) and the surrounding molecular envelope (in the 1-0 S(1) line of H-2). The observations show that the ionized gas forms an elongated (similar to6 x 12, PA = 32degrees), limb-brightened shell with an expansion velocity of 19.5 km s(-1) along the line of sight. The shell is composed of numerous small condensations and has nearly parallel sides with flattened ends that are not well matched by a uniform ellipsoidal model. Low level Brgamma emission is detected at high red- and blue-shifted velocities (+/-55 km s(-1)) along a bipolar axis at PA = 60degrees that deviates significantly from that of the main nebula. The H2 emission is distributed at the periphery of the ionized gas, in a limb-brightened, bi-conical shell (similar to10 x 13, PA = 28degrees) with enhanced emission at the equator and complex structure at the ends of the major axis. The H2 emission traces the inner edge of the extended molecular envelope seen in CO, and its distribution and intensity are well matched by model predictions of a high-density (n(H) similar to 10(6)-10(5) cm(-3)) photo-dissociation region. The kinematic structure of the H-2 emission reveals a remarkable series of lobes and openings in the molecular shell. These features are point symmetric about the center, and the most prominent pair aligns with the high velocity, bipolar emission seen in Brgamma. These observations demonstrate recent activity by collimated outflows in NGC 7027, with a multiple, bipolar geometry. The interaction of the outflows with the surrounding envelope has significantly affected the morphology of the developing nebula and its environment, and their presence in this well-studied archetype underscores the general importance of outflows in the early shaping history of planetary nebulae.