The circumnuclear star formation environment of NGC 6946: Br γ and H2 results from keck integral field spectroscopy

Abstract

We present a three-dimensional data cube of the K-band continuum and the Br γ, H2 S(0), and S(1) lines within the central 18.″5 × 13.″8 (520 pc × 390 pc) region of NGC 6946. Data were obtained using OSIRIS, a near-infrared Integral Field Spectrograph at Keck Observatory, with Laser Guide Star Adaptive Optics. The 0.″3 resolution allows us to investigate the stellar bulge and the forming star clusters in the nuclear region on 10 pc scales. We detect giant H II regions associated with massive young star clusters in the nuclear spiral/ring (R 30 pc) and in the principal shocks along the nuclear bar. Comparisons of the Br γ fluxes with Pa α line emission and radio continuum indicate AK 3, AV 25 for the nuclear star-forming regions. The most luminous H II regions are restricted to within 70 pc of the center, despite the presence of high gas columns at larger radii (R 200 pc). H2 emission is restricted to clouds within R 60 pc of the center, resembling the distribution of HCN line emission. We propose that gas-assisted migration of the young star clusters is contributing to the buildup of the nuclear bar and nuclear star cluster (R < 30 pc) in this galaxy. © 2013. The American Astronomical Society. All rights reserved.