2021A&A...648A..61B


Query : 2021A&A...648A..61B

2021A&A...648A..61B - Astronomy and Astrophysics, volume 648A, 61-61 (2021/4-1)

Infrared action spectroscopy of doubly charged PAHs and their contribution to the aromatic infrared bands.

BANHATTI S., PALOTAS J., JUSKO P., REDLICH B., OOMENS J., SCHLEMMER S. and BRUNKEN S.

Abstract (from CDS):

The so-called aromatic infrared bands (AIBs) are attributed to emission of polycyclic aromatic hydrocarbons (PAHs). The observed variations toward different regions in space are believed to be caused by contributions of different classes of PAH molecules, that is to say with respect to their size, structure, and charge state. Laboratory spectra of members of these classes are needed to compare them to observations and to benchmark quantum-chemically computed spectra of these species. In this paper we present the experimental infrared (IR) spectra of three different PAH dications, naphthalene2+, anthracene2+, and phenanthrene2+, in the vibrational fingerprint region 500-1700cm–1. The dications were produced by electron impact ionization of the vapours with 70 eV electrons, and they remained stable against dissociation and Coulomb explosion. The vibrational spectra were obtained by IR predissociation of the PAH2+ complexed with neon in a 22-pole cryogenic ion trap setup coupled to a free-electron infrared laser at the Free-Electron Lasers for Infrared eXperiments (FELIX) Laboratory. We performed anharmonic density-functional theory calculations for both singly and doubly charged states of the three molecules. The experimental band positions showed excellent agreement with the calculated band positions of the singlet electronic ground state for all three doubly charged species, indicating its higher stability over the triplet state. The presence of several strong combination bands and additional weaker features in the recorded spectra, especially in the 10-15µm region of the mid-IR spectrum, required anharmonic calculations to understand their effects on the total integrated intensity for the different charge states. These measurements, in tandem with theoretical calculations, will help in the identification of this specific class of doubly-charged PAHs as carriers of AIBs.

Abstract Copyright: © ESO 2021

Journal keyword(s): ISM: lines and bands - ISM: molecules - techniques: spectroscopic - methods: laboratory: molecular - molecular data - line: identification

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NAME Orion Bright Bar reg 05 35 22.30 -05 24 33.0           ~ 863 0
2 HD 44179 pA* 06 19 58.2185496 -10 38 14.706068 9.51 9.33 9.02     B9Ib/II 761 0
3 NGC 7023 RNe 21 01 36.9 +68 09 48           ~ 702 0

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