SIMBAD references

The energy sources of nine infrared luminous galaxies (IRLGs) are diagnosed based on their ground-based 3-4 µm spectra. Both the equivalent width of the 3.3 µm polycyclic aromatic hydrocarbon (PAH) emission feature and the 3.3 µm PAH to far-infrared luminosity ratio (L_3.3/L_FIR) are analyzed. Assuming that nuclear compact starburst activity in these sources produces the 3.3 µm PAH emission as strongly as that in starburst galaxies with lower far-infrared luminosities, the following results are found. For six IRLGs, both the observed equivalent widths and the L_3.3/L_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 µm PAH equivalent widths are within the range of starburst galaxies, the L_3.3/L_FIR ratios after correction for screen dust extinction are a factor of ∼3 smaller. The uncertainty in the dust extinction correction factor and in the scatter of the intrinsic L_3.3/L_FIR ratios for starburst galaxies does not allow a determination of the ultimate energy sources for these three IRLGs.