Detection and mapping of decoupled stellar and ionized gas structures in the ultraluminous infrared galaxy IRAS 12112+0305

Integral field optical spectroscopy with the INTEGRAL fiber-fed system and Hubble Space Telescope optical imaging are used to map the complex stellar and warm ionized gas structure in the ultraluminous infrared galaxy IRAS 12 112+0305. Images reconstructed from wavelength-delimited extractions of the integral field spectra reveal that the observed ionized gas distribution i s decoupled from the stellar main body of the galaxy, with the dominant con tinuum and emission-line regions separated by projected distances of up to 7.5 kpc. The two optical nuclei are detected as apparently faint emission-l ine regions, and their optical properties are consistent with being dust-en shrouded weak [O (I)] LINERs. The brightest emission-line region is associa ted with a faint (m(I) = 20.4), giant H (II) region of 600 pc diameter, in which a young (similar to 5 Myr) massive cluster of about 2 x 10(7) M. domi nates the ionization. Internal reddening toward the line-emitting regions a nd the optical nuclei ranges from 1 to 8 mag in the visual. Taking the redd ening into account, the overall star formation in IRAS 12112+0305 is domina ted by starbursts associated with the two nuclei and corresponds to a star formation rate of 80 M. yr(-1).