The energetics of acetylene loss from the naphthalene cation and the r
elative stabilities of the three most probable cationic fragments have
been investigated using the CIPSI method and CASSCF plus CI treatment
s. Theoretical results, which are in agreement with experimental data
when available, point to the benzocyclobutadiene cation as a possible
product of polycyclic aromatic hydrocarbon (PAH) fragmentation in the
interstellar medium.