H. Cottin et al., Production of hexamethylenetetramine in photolyzed and irradiated interstellar cometary ice analogs, ASTROPHYS J, 561(1), 2001, pp. L139-L142
We report hexamethylenetetramine (HMT) detection in organic residues result
ing from H2O : CO : CH3OH : NH3 ices submitted to UV photolysis or proton i
rradiation. This is the first time HMT is detected after proton irradiation
of an interstellar or cometary ice analog, whereas this molecule was suspe
cted to be a characteristic signature of UV versus ion processing. This res
ult strengthens the probability of HMT presence in the interstellar medium
and in comets, where it may eventually be detected with the COSAC (COmetary
Sampling And Composition) experiment on board the upcoming Rosetta mission
.