Photolysis of interstellar ice analogs containing ethanol: A new approach to forming C2H4O2 isomers

Open Access

Fig. 3

IR spectra, between 2400 and 500 cm ¹, of pure CH₃CH₂OH ice at 10 K before (b) and after (c) UV irradiation. Spectrum (a), taken from NASA cosmic ice laboratory (Hudson et al. 2009), shows the CH₃CHO:H₂O ice.

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