Cosmic-ray-induced chemical processes in CH3OH, CH3NH2, and CH3OH:CH3NH2 ices - Conventional and novel IR spectroscopic analysis with VIZSLA

Open Access

Fig. 3

Difference spectrum of electron bombarded CH₃OH:CH₃NH₂ ice at 3 K, zoomed in on key spectral bands. The difference spectrum was obtained by subtracting the MIR spectrum recorded after the electron bombardment from the spectrum recorded after the deposition.

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