“…However, for pericondensed PAHs, including pyrene, loss of C 2 H 2 is inhibited because a key transition state is too high in energy. 10 Indeed, experiments reveal that for PAHs in the astrophysically-relevant size range (50-100 carbon atoms), fragmentation is dominated by hydrogen-loss until mostif not all -hydrogen atoms are lost. 8,10,11 For completeness, we mention that in regions with high atomic hydrogen density and low UV fields, interstellar PAHs can be superhydrogenated (i.e.…”