F. Hoyle et Nc. Wickramasinghe, A unified model for the 3.28 mu emission and the 2200 angstrom interstellar extinction feature, ASTRO SP SC, 268(1-3), 1999, pp. 305-310
The 3.28 mu m feature observed in the diffuse galactic emission and the 220
0 Angstrom interstellar extinction feature must have a common source. This
requirement rules out graphitic-type PAH molecules such as coronone and ten
ds to favour naturally occurring bi-cyclic ring structures typified by quin
oline and its derivatives.