The Profiles of the 3-12 Micron Polycyclic Aromatic Hydrocarbon Features

By B. Diedenhoven, E. Peeters, C. V. Kerckhoven, S. Hony, D. Hudgins, L. Allamandola, A. Tielens. 2004

208 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/c7cc1a4ab4bffff35fc5fae811db317bfa254d0d

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

Citations in the corpus

Variations of the Mid-IR Aromatic Features inside and among Galaxies (2008, background): “It is asymmetric and varies as a function of environment (e.g., Peeters et al. 2002b; van Diedenhoven et al. 2004).”
The Infrared Spectra of Very Large, Compact, Highly Symmetric, Polycyclic Aromatic Hydrocarbons (PAHs) (2008, background): “3 by van Diedenhoven et al. (2004) reflect the relative contributions of PAH neutrals and anions.”
Polycyclic Aromatic Hydrocarbons as a Tracer of Star Formation? (2004, background): “…are very similar, the individual sources display great diversity in their spectral properties (for this sample see Roelfsema et al. 1996; Verstraete et al. 1996, 2001; Hony et al. 2001; Peeters et al. 2002a, 2002b; Martı́n-Hernández et al. 2002; Vermeij et al. 2002; van Diedenhoven et al. 2004).”
C2D Spitzer-IRS spectra of disks around T Tauri stars. II. PAH emission features (2006, background): “…a previous study of a diverse sample of interstellar and circumstellar sources, planetary nebulae, reflection nebulae HII regions and galaxies (van Diedenhoven et al. 2004), the 11.2µm PAH feature of almost all YSO’s, non-isolated HAeBe stars and HII regions was found to have a similar asymmetric…”
The Behavior of the Aromatic Features in M101 H II Regions: Evidence for Dust Processing (2008, background): “…of Toledo, Toledo, OH 43603 4 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK gle sources (Werner et al. 2004), among various Galactic sources (van Diedenhoven et al. 2004), and among galaxies (Engelbracht et al. 2005; Madden et al. 2006; Wu et al. 2006).”
THE NASA AMES POLYCYCLIC AROMATIC HYDROCARBON INFRARED SPECTROSCOPIC DATABASE: THE COMPUTED SPECTRA (2010, unknown): “…in the emitting regions and the nature of the PAH carriers (e.g., Joblin et al. 1994; Li & Draine 2001; Hony et al. 2001; Peeters et al. 2002; van Diedenhoven et al. 2004; Mulas et al. 2006; Bauschlicher et al. 2008, 2009; Galliano et al. 2008; Boersma et al. 2009, 2010; Mattioda et al. 2009;…”
THE INFRARED SPECTRA OF VERY LARGE IRREGULAR POLYCYCLIC AROMATIC HYDROCARBONS (PAHs): OBSERVATIONAL PROBES OF ASTRONOMICAL PAH GEOMETRY, SIZE, AND CHARGE (2009, methodology): “A detailed analysis of the astronomical features produced by the aromatic CH stretching (CHstr) vibrations was given by van Diedenhoven et al. (2004).”