Direct observation of long-lived cyanide anions in superexcited states.

The cyanide anion (CN - ) has been identified in cometary coma, interstellar medium, planetary atmosphere and circumstellar envelopes, but its origin and abundance are still disputed. An isolated CN - is stabilized in the vibrational states up to ν = 17 of the electronic ground-state 1 Σ + , but it is not thought to survive in the electronic or vibrational states above the electron autodetachment threshold, namely, in superexcited states. Here we report the direct observation of long-lived CN - yields of the dissociative electron attachment to cyanogen bromide (BrCN), and confirm that some of the CN - yields are distributed in the superexcited vibrational states ν ≥ 18 ( 1 Σ + ) or the superexcited electronic states 3 Σ + and 3 Π. The triplet state can be accessed directly in the impulsive dissociation of BrCN - or by an intersystem transition from the superexcited vibrational states of CN - . The exceptional stability of CN - in the superexcited states profoundly influences its abundance and is potentially related to the production of other compounds in interstellar space.