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Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds

Space Sciences

Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds

M. H. Stockett, J. N. Bull, et al.

This groundbreaking research by Mark H. Stockett and colleagues reveals that the abundance of cyanonaphthalene in the Taurus Molecular Cloud far exceeds expectations, challenging existing astrophysical models. The study uncovers critical insights into the stability of 1-CNN⁺ and its implications for the understanding of small PAH destruction in space.

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