Gas-phase infrared spectra of hydrogenated and methylated pyrenes, combined with a Monte Carlo cooling model, point to 1,2,3,6,7,8-hexahydropyrene as the carrier of the 3.403 μm component of the interstellar 3.4 μm emission band.
Physical Chemistry Chemical Physics (Incorporating Faraday Transactions) , year = 2011, month = jan, volume =
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Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 $\mu$m emission band
Gas-phase infrared spectra of hydrogenated and methylated pyrenes, combined with a Monte Carlo cooling model, point to 1,2,3,6,7,8-hexahydropyrene as the carrier of the 3.403 μm component of the interstellar 3.4 μm emission band.