Imaging of ultraluminous infrared galaxies in the near-ultraviolet

We present the first ground-based U' (lambda(central) = 3410 Angstrom, Delt a(lambda) = 320 Angstrom) images of ultraluminous infrared galaxies (ULIGs) . Two samples were observed: (1) "warm" ULIGs with mid-infrared colors char acteristic of active galactic nuclei (f(25 mu m)/f(60 mu m) > 0.2), which a re believed to represent a critical transition phase between cooler ULIGs a nd optically selected QSOs according to a previously proposed evolutionary model, and (2) the complementary "cool" ULIGs (f(25 mu m)/f(60 mu m) < 0.2) , which in the evolutionary model are the progenitors of warm ULIGs and whi ch have many characteristics associated with active star formation. Althoug h in some cases there is also emission identified with an active galactic n ucleus, the U' emission originates primarily in massive young stars and as such allows a direct examination of the sites of recent high-mass star form ation. Strong U' emission (median total M-U = -20.8) is seen in all systems , and in some cases the extended tidal features (both the smooth stellar di stribution and compact star-forming features) contribute up to 60%-80% of t he total flux. The star-forming regions in both samples are found to have a ges based on spectral synthesis models in the range 10-100 Myr, and most di fferences in color between them can be attributed to the effects of dust re ddening. Additionally, it is found that star formation in compact knots in the tidal tails is most prominent in those ULIGs that have double nuclei, s uggesting that the star formation rate in the tails peaks prior to the actu al coalescence of the galaxy nuclei and diminishes quickly thereafter. Simi lar to results at other wavelengths, the observed star formation at U' can account for only a small fraction of the known bolometric luminosity of the ULIGs. Azimuthally averaged radial light profiles at U' are characterized by a SBrsic law with index n = 2, which is intermediate between an exponent ial disk and an r(-1/4) law and closely resembles the latter at large radii . The implications of this near-ultraviolet imaging for optical/near-infrar ed observations of high-redshift counterparts of ULIGs are discussed.