Energy Diagnoses of Nine Infrared Luminous Galaxies Based on 3--4 Micron Spectra

The energy sources of nine infrared luminous galaxies (IRLGs) are diagnosed based on their ground-based 3--4 $\\mu$m spectra. Both the equivalent width of the 3.3 $\\mu$m polycyclic aromatic hydrocarbon (PAH) emission feature and the 3.3 $\\mu$m PAH to far-infrared luminosity ratio ($L_{3.3}/L_{\\rm FIR}$) are analyzed. Assuming nuclear compact starburst activity in these sources produces the 3.3 $\\mu$m PAH emission as strongly as that in starburst galaxies with lower far-infrared luminosities, the followings results are found: For six IRLGs, both the observed equivalent widths and the $L_{3.3}/L_{\\rm FIR}$ ratios are too small to explain the bulk of their far-infrared luminosities by compact starburst activity, indicating that active galactic nucleus (AGN) activity is a dominant energy source. For the other three IRLGs, while the 3.3 $\\mu$m PAH equivalent widths are within the range of starburst galaxies, the $L_{3.3}/L_{\\rm FIR}$ ratios after correction for screen dust extinction are a factor of $\\sim$3 smaller. The uncertainty in the dust extinction correction factor and in the scatter of the intrinsic $L_{3.3}/L_{\\rm FIR}$ ratios for starburst galaxies do not allow a determination of the ultimate energy sources for these three IRLGs.