The rich 6 to 9m spectrum of interstellar PAHs
By E. Peeters, S. Hony, L. Allamandola, D. Hudgins, C. Bauschlicher. 2002
166 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/4138f29b9f5f3527be312955e7d751f741cdf771
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- A. Tielens
- F. Galliano
- S. Madden
- E. Peeters
- J. Oomens
- A. Jones
- B. Sartakov
- G. Helden
Citations in the corpus
- Laboratory Infrared Spectroscopy of Cationic Polycyclic Aromatic Hydrocarbon Molecules (2003, methodology): “…galactic nuclei, and starburst galaxies (Verstraete et al. 1996, 2001; Moutou et al. 1999; Joblin et al. 2000; Genzel et al. 1998; Henning et al. 1998; Boulanger et al. 1998; Mattila et al. 1996; Mattila, Lehtinen, & Lemke 1999; van Kerckhoven et al. 2000; Hony et al. 2001; Peeters et al. 2002).”
- Variations of the Mid-IR Aromatic Features inside and among Galaxies (2008, background): “PAH VARIATIONS INSIDE AND AMONG GALAXIES 311 1999), and the Orion Bar (Cesarsky et al. 2000), and the ISO SWS spectra (2.5Y45 m) of several compact H ii regions published by Peeters et al. (2002a).”