The formation of nitrogen-containing organic compounds
is crucial
for understanding chemical evolution and the origin of life in the
interstellar medium (ISM). In this study, we explore whether acrylonitrile
(AN) and pyrrole (Py) can form new nitrogen-containing compounds after
single-photon ionization in their gaseous clusters by vacuum ultraviolet
(VUV)-infrared (IR) spectroscopy and theoretical calculations. The
results show that a strong linear H-bond is formed in neutral AN-Py,
while cyclic or bicyclic H-bonded networks are formed in the neutral
AN-Py2 cluster. It is found that the structure containing
a new C–C covalent bond between two moieties in (AN-Py)+ is formed besides the formation of H-bonded structures after
AN-Py is ionized by VUV light. In (AN-Py2)+ cluster
cations, new C–C or C–N covalent bonds tend to be formed
between two Py, with (Py)2+ as the core in the
cluster. The results reveal that new covalent bonds are more likely
to be formed between two Py species when AN and Py are present in
the cationic clusters. These results provide spectroscopic evidence
of the formation of new nitrogen-containing organic compounds from
AN and Py induced by VUV, which are helpful for our understanding
of the formation of diverse prebiotic molecules in interstellar space