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Modeling the Unidentified Infrared Emission with Combinations of Polycyclic Aromatic Hydrocarbons

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Allamandola, L. J., Hudgins, D. M., Sandford, S. A.·1999·The Astrophysical Journal

Abstract

The infrared emission band spectrum associated with many different interstellar objects can be modeled successfully by using combined laboratory spectra of neutral and positively charged polycyclic aromatic hydrocarbons (PAHs). These model spectra, shown here for the first time, alleviate the principal spectroscopic criticisms previously leveled at the PAH hypothesis and demonstrate that mixtures of free molecular PAHs can indeed account for the overall appearance of the widespread interstellar infrared emission spectrum. Furthermore, these models give us insight into the structures, stabilities, abundances, and ionization balance of the interstellar PAH population. These, in turn, reflect conditions in the emission zones and shed light on the microscopic processes involved in the carbon nucleation, growth, and evolution in circumstellar shells and the interstellar medium.

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Metadata

Authors
Allamandola, L. J., Hudgins, D. M., & Sandford, S. A.
Venue
The Astrophysical Journal
Published
1999-02-01
Volume
511
Issue
2
Pages
L115-L119
ISSN
0004-637X (ISSN-L)
OpenAlex
W2097527096
Cited by
452
References
0
FWCI
15.72
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Modeling the Unidentified Infrared Emission with Combinations of Polycyclic Aromatic Hydrocarbons. https://app.cochat.ai/papers/10.1086/311843
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Allamandola, L. J., Hudgins, D. M., & Sandford, S. A. (1999). Modeling the Unidentified Infrared Emission with Combinations of Polycyclic Aromatic Hydrocarbons. The Astrophysical Journal. https://doi.org/10.1086/311843

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.