4.7 Article

HIGH-RESOLUTION IR ABSORPTION SPECTROSCOPY OF POLYCYCLIC AROMATIC HYDROCARBONS IN THE 3 μm REGION: ROLE OF PERIPHERY

期刊

ASTROPHYSICAL JOURNAL
卷 831, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.3847/0004-637X/831/1/58

关键词

astrochemistry; ISM: molecules; line: identification; methods: laboratory: molecular; techniques: spectroscopic

资金

  1. Netherlands Organization for Scientific Research (NWO)
  2. NWO [723.014.007, 639.041.543]
  3. Advanced European Research Council [246976]
  4. Spinoza award
  5. NWO Exacte Wetenschappen [MP-270-13, MP-264-14]
  6. NASA [12-APRA12-0107]
  7. NASA/SETI [NNX15AF45A]
  8. National Aeronautics and Space Administration through the NASA Astrobiology Institute [NNH13ZDA017C]
  9. European Research Council (ERC) [246976] Funding Source: European Research Council (ERC)
  10. NASA [803838, NNX15AF45A] Funding Source: Federal RePORTER

向作者/读者索取更多资源

In this work we report on high-resolution IR absorption studies that provide a detailed view on how the peripheral structure of irregular polycyclic aromatic hydrocarbons (PAHs) affects the shape and position of their 3 mu m absorption band. For this purpose, we present mass-selected, high-resolution absorption spectra of cold and isolated phenanthrene, pyrene, benz[a]antracene, chrysene, triphenylene, and perylene molecules in the 2950-3150 cm(-1) range. The experimental spectra are compared with standard harmonic calculations and anharmonic calculations using a modified version of the SPECTRO program that incorporates a Fermi resonance treatment utilizing intensity redistribution. We show that the 3 mu m region is dominated by the effects of anharmonicity, resulting in many more bands than would have been expected in a purely harmonic approximation. Importantly, we find that anharmonic spectra as calculated by SPECTRO are in good agreement with the experimental spectra. Together with previously reported high-resolution spectra of linear acenes, the present spectra provide us with an extensive data set of spectra of PAHs with a varying number of aromatic rings, with geometries that range from open to highly condensed structures, and featuring CH groups in all possible edge configurations. We discuss the astrophysical implications of the comparison of these spectra on the interpretation of the appearance of the aromatic infrared 3 mu m band, and on features such as the two-component emission character of this band and the 3 mu m emission plateau.

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