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Hudgins DM, Allamandola LJ 
The spacing of the interstellar 6.2 and 7.7 micron emission features as an indicator of polycyclic aromatic hydrocarbon size. [Journal Article]
Astrophys J 1999 Mar 1; 513(1 Pt 2):L69-73.
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Allamandola LJ, Tielens AG, Barker JR 
Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications. [Journal Article, Review]
Astrophys J Suppl Ser 1989 Dec.:733-75.
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Hudgins DM, Allamandola LJ 
Interstellar PAH emission in the 11-14 micron region: new insights from laboratory data and a tracer of ionized PAHs. [Journal Article]
Astrophys J 1999 May 1; 516(1 Pt 2):L41-4.
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Salama F, Bakes EL, Allamandola LJ, et al. 
Assessment of the polycyclic aromatic hydrocarbon-diffuse interstellar band proposal. [Journal Article]
Astrophys J 1996 Feb 20; 458(2 Pt 1):621-36.
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Allamandola LJ, Bregman JD, Sandford SA, et al. 
The discovery of a new infrared emission feature at 1905 wavenumbers (5.25 microns) in the spectrum of BD +30 degrees 3639 and its relation to the polycyclic aromatic hydrocarbon model. [Journal Article]
Astrophys J 1989 Oct 1; 345(1):L59-62.
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Hudgins DM, Allamandola LJ, Sandford SA 
Complex organic molecules in space: the carriers of the interstellar infrared emission features. [Journal Article]
Adv Space Res 1997; 19(7):999-1008.
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Hudgins DM, Allamandola LJ 
Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon cations. 3. The polyacenes anthracene, tetracene, and pentacene. [Journal Article, Research Support, U.S. Gov't, Non-P.H.S. ]
J Phys Chem 1995 Jun 1; 99(22):8978-86.
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Witteborn FC, Sandford SA, Bregman JD, et al. 
New emission features in the 11-13 micron region and their relationship to polycyclic aromatic hydrocarbons. [Journal Article]
Astrophys J 1989 Jun 1; 341(1):270-7.
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Cook DJ, , Schlemmer S, Balucani N, et al. 
Infrared emission spectra of candidate interstellar aromatic molecules. [Journal Article]
Nature 1996 Mar 21; 380(6571):227-9.
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