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2018ApJ...854...27Z - Astrophys. J., 854, 27-27 (2018/February-2)

Laboratory gas-phase infrared spectra of two astronomically relevant PAH cations: diindenoperylene, C32H16+ and dicoronylene, C48H20+.

ZHEN J., CANDIAN A., CASTELLANOS P., BOUWMAN J., LINNARTZ H. and TIELENS A.G.G.M.

Abstract (from CDS):

The first gas-phase infrared spectra of two isolated astronomically relevant and large polycyclic aromatic hydrocarbon (PAH) cations-diindenoperylene (DIP) and dicoronylene (DC)-in the 530-1800 cm–1 (18.9-5.6 µm) range-are presented. Vibrational band positions are determined for comparison to the aromatic infrared bands. The spectra are obtained via infrared multiphoton dissociation spectroscopy of ions stored in a quadrupole ion trap using the intense and tunable radiation of the free electron laser for infrared experiments (FELIX). DIP+ shows its main absorption peaks at 737 (13.57), 800 (12.50), 1001 (9.99), 1070 (9.35), 1115 (8.97), 1152 (8.68), 1278 (7.83), 1420 (7.04), and 1550 (6.45) cm–1(µm), in good agreement with density functional theory (DFT) calculations that are uniformly scaled to take anharmonicities into account. DC+ has its main absorption peaks at 853 (11.72), 876 (11.42), 1032 (9.69), 1168 (8.56), 1300 (7.69), 1427 (7.01), and 1566 (6.39) cm–1(µm), which also agree well with the scaled DFT results presented here. The DIP+ and DC+ spectra are compared with the prominent infrared features observed toward NGC 7023. This results both in matches and clear deviations. Moreover, in the 11.0-14.0 µm region, specific bands can be linked to CH out-of-plane (oop) bending modes of different CH edge structures in large PAHs. The molecular origin of these findings and their astronomical relevance are discussed.

Abstract Copyright: © 2018. The American Astronomical Society.

Journal keyword(s): astrochemistry - ISM: abundances - ISM: molecules - molecular data - molecular processes

Simbad objects: 1

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