Laboratory Infrared Spectroscopy of Cationic Polycyclic Aromatic Hydrocarbon Molecules
By J. Oomens, A. Tielens, B. Sartakov, G. Helden, G. Meijer. 2003
202 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/4a26017e756615f1ab851f2e7817c8f069b36bcc
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- E. Peeters
- A. Tielens
- L. Allamandola
- C. Bauschlicher, Jr.
- D. Hudgins
- S. Hony
- C. Bauschlicher
- E. Dishoeck
In Atomic and Molecular Physics, and Optics
In Spectroscopy
- E. Peeters
- A. Tielens
- L. Allamandola
- C. Bauschlicher, Jr.
- E. Dishoeck
- B. Draine
- C. Bauschlicher
- S. Glover
Citations in the corpus
- The Profiles of the 3-12 Micron Polycyclic Aromatic Hydrocarbon Features (2004, background): “…from laboratory studies on the temperature dependence of the peak wavelength and width of the absorption bands (Joblin et al. 1995) and from the difference between low-temperature absorption measurements and infrared multiphoton dissociation studies of trapped PAH ions (Oomens et al. 2003).”
- Variations in the Peak Position of the 6.2 μm Interstellar Emission Feature: A Tracer of N in the Interstellar Polycyclic Aromatic Hydrocarbon Population (2005, background): “…(e.g., Hudgins et al. 2000; Vala et al. 1994; Szczepanski et al. 1995; Bauschlicher & Langhoff 1997; Kim & Saykally 2002; Mattioda et al. 2003; Oomens et al. 2003 and references therein), it is now widely recognized that models based on the composite spectra of PAHs and PAH cations can…”