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HIZOA J0836-43is one of the most HI-massive galaxies in the local (z<0.1)Universe. Not only are such galaxies extremely rare, but this "coelacanth"galaxy exhibits characteristics -- in particular its active, inside-out stellardisk-building -- that appear more typical of past (z ~ 1) star formation, whenlarge gas fractions were more common. Unlike most local giant HI galaxies, itis actively star forming. Moreover, the strong infrared emission is not inducedby a merger event or AGN, as is commonly found in other local LIRGs. The galaxyis suggestive of a scaled-up version of local spiral galaxies; its extendedstar formation activity likely being fueled by its large gas reservoir and, assuch, can aid our understanding of star formation in systems expected todominate at higher redshifts. The multi-wavelength imaging and spectroscopicobservations that have led to these deductions will be presented. These includeNIR (J H K) and MIR (Spitzer; 3-24micron) imaging and photometry, MIRspectroscopy, ATCA HI-interferometry and Mopra CO line emission observations.But no optical data, as the galaxy is heavily obscured due to its location inVela behind the Milky Way.

The SED of the nearby HI-massive LIRG HIZOA J0836-43: from the NIR to the radio domain