Adaptive optics observations of luminous infrared galaxies. II. Imaging of the merging galaxy Arp 299

Abstract

We present adaptive optics observations of the Luminous Infrared Galaxy, Arp 299. This merging galaxy (NGC 3690) is the site of a very powerful starburst activity. Very high angular resolution observations at 2.2mic reveal many super-clusters of newly formed stars. Those clusters feature intrinsic luminosities and surface densities well above the figures generally found in the Local Cluster, pointing to a highly efficient stellar formation with possibly very high mass stars. Comparison with hst images in V band allows us to extract a [V-K] map, and shows that the extinction varies largely within the area. Comparison of the very nucleus of Mkn 171A to a model point spread function shows that it is resolved in K band, with a FWHM of 0.4arcsec leading to the conclusion that an AGN as the primary power source is very unlikely. The small size, high extinction and high intrinsic luminosity of this nucleus prompts us to suggest an ultra-compact starburst as primary source of luminosity. Based on observations obtained at the Canada--France--Hawaii Telescope operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique and the University of Hawaii.