Simulated Infrared Emission Spectra of Highly Excited Polyatomic Molecules: A Detailed Model of the PAH‐UIR Hypothesis

Author:

Cook D. J.,Saykally R. J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference36 articles.

1. The discovery of a new infrared emission feature at 1905 wavenumbers (5.25 microns) in the spectrum of BD + 30 deg 3639 and its relation to the polycyclic aromatic hydrocarbon model

2. Allamandola, L. J., Sandford, S. A., Hudgins, D. M. & Witteborn, F. C. 1995, in ASP Conf. Proc. 73, Airborne Astron. Symp. Galactic Ecosystem, ed. M. R. Haas, J. A. Davidson & E. F. Erickson (San Francisco: ASP), 23

3. Polycyclic aromatic hydrocarbons and the unidentified infrared emission bands - Auto exhaust along the Milky Way

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