NEUTRAL AND IONIZED POLYCYCLIC AROMATIC-HYDROCARBONS, DIFFUSE INTERSTELLAR BANDS AND THE ULTRAVIOLET EXTINCTION CURVE

Neutral naphthalene (C10H8), phenanthrene (C14H10) and pyrene (C16H10) absorb strongly in the ultraviolet region and may contribute to the extinction curve. High abundances are required to produce detectable structures. The cations of these polycyclic aromatic hydrocarbons (PAHs) absorb in the visible. C10H8+ has 13 discrete absorption bands which fall between 6800 and 4500 angstrom. The strongest band at 6741 angstrom falls close to the weak 6742 angstrom diffuse interstellar band (DIB) Five other weaker bands also match DIBs. The possibility that C10H8+ is responsible for some of the DIBs can be tested by searching for new DIBs at 6520 and 6151 angstrom, other strong naphthalene cation band positions. If C10H8+ is indeed responsible for the 6742 angstrom feature, it accounts for 0.3% of the cosmic carbon. The spectrum of C16H10+ is dominated by a strong band at 4435 angstrom in an Ar matrix and 4395 angstrom in Ne, wavelengths which fall very close to the strongest DIB at 4430 angstrom. If C16H10+, or a closely related pyrene-like ion, is indeed responsible for the 4430 angstrom feature, it accounts for 0.2% of the cosmic carbon. An intense, very broad UV-to-visible continuum is reported which is associated with both ions and could explain how PAHs convert interstellar UV and visible radiation into IR radiation.