Spectroscopy and Photochemistry of [Al, N, C, O, H]: Connectivity to Aluminium‐Bearing Species in the Universe

Abstract

Aluminium is one of the most abundant metals in the universe and impacts the evolution of various astrophysical environments. Currently detected Al‐bearing molecules represent only a small fraction of the aluminium budget, suggesting that aluminium may reside in other species. AlO and AlOH molecules are abundant in the oxygen‐rich supergiant stars such as VY Canis Majoris, a stellar molecular factory with 60+ molecules including the prebiotic NC‐bearing species. Additional Al‐bearing molecules with N, C, O, and H may form in O‐rich environments with radiation‐accelerated chemistry. Here, we present spectroscopic identification of novel aluminium‐bearing molecules composed of [Al, N, C, O, H] and [Al, N, C, O] from the reactions of Al atoms and HNCO in solid argon matrix, which are potential Al‐bearing molecules in space. Photoinduced transformations among six [Al, N, C, O, H] isomers and three [Al, N, C, O] isomers, along with their dissociation reactions forming the known interstellar species, have been disclosed. These results provide new insight into the chemical network of astronomically detected Al‐bearing species in space.