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- W2110132255 abstract "We present adaptive optics observations of the Lu- minous Infrared Galaxy, Arp 299. This merging galaxy (NGC 3690) is the site of a very powerful starburst activity. Very high angular resolution observations at 2.2m reveal many super- clusters of newly formed stars. Those clusters feature intrinsic luminosities and surface densities well above the figures gen- erally found in the Local Cluster, pointing to a highly efficient stellar formation with possibly very high mass stars.Compar- ison 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 of0:4 00 leading to the conclusion that an AGN as the primary power source is very unlikely. The small size, high ex- tinction and high intrinsic luminosity of this nucleus prompts us to suggest an ultra-compact starburst as primary source of luminosity." @default.
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- W2110132255 date "1999-11-01" @default.
- W2110132255 modified "2023-09-26" @default.
- W2110132255 title "Adaptive optics observations of luminous infrared galaxies II. Imaging of the merging galaxy Arp 299" @default.
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