“…We find that, first, NO tends to adsorb on the niobium clusters via the N–Nb bonding, and the N–O bond can be spontaneously dissociated for all four studied systems within the 0.1–10 ps time scale, which means collisional stabilization of helium can be ignored (For more details on other clusters, see Figure S29, ESI.). This is accessible with a low energy barrier of the transition states (TS) which result from the formation of N/O binding onto the Nb atoms. , The reactivity of the single atomic cation Nb + follows the free radical mechanism just like the other transition metal ions such as Sc, Ti, and V, ,− whereas the dissociatively adsorbed Nb n NO + clusters will allow for Nb–Nb bond cleavage (to form Nb n –1 N + or Nb n –1 O + ) along with NbO/NbN loss. For the relatively larger cluster Nb 10 + , the N atom forms hollow site binding with an energy gain of 2.99 eV which allows for the subsequent dissociation reaction.…”