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most citedThe rich 6 to 9 um spectrum of interstellar PAHs

643 citations · 3.7k across the 50 of their papers we have counts for

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astro-ph2008★ 61 cited

The 5.25 & 5.7 m Astronomical Polycyclic Aromatic Hydrocarbon Emission Features

C. Boersma, A. L. Mattioda, C. W. Bauschlicher +3

Astronomical mid-IR spectra show two minor PAH features at 5.25 and 5.7 m (1905 and 1754 cm) that hitherto have been little studied, but contain information about th…

astro-ph2008★ 6 cited

A mid-infrared study of HII regions in the Magellanic Clouds: N88A and N160A

N. L. Martin-Hernandez, E. Peeters, A. G. G. M. Tielens

To show the importance of high-spatial resolution observations of HII regions when compared with observations obtained with larger apertures such as ISO, we present mid-infrared sp…

astro-ph2008★ 196 cited

The infrared spectra of very large, compact, highly symmetric, polycyclic aromatic hydrocarbons (PAHs)

Charles W. Bauschlicher, Els Peeters, Louis J. Allamandola

The mid-infrared spectra of large PAHs ranging from C54H18 to C130H28 are determined computationally using Density Functional Theory. Trends in the band positions and intensities a…

astro-ph2008★ 299 cited

Variations of the Mid-IR Aromatic Features Inside and Among Galaxies

F. Galliano, S. C. Madden, A. G. G. M. Tielens +2

We present the results of a systematic study of mid-IR spectra of Galactic regions, Magellanic HII regions, and galaxies of various types (dwarf, spiral, starburst), observed by th…

astro-ph2006★ 67 cited

The Spitzer-IRS spectrum of SMP LMC 11

J. Bernard-Salas, E. Peeters, G. C. Sloan +3

We present the first mid-infrared spectra of SMP LMC 11 in the Large Magellanic Cloud. While this object resembles a planetary nebula in the optical, its infrared properties are mo…

astro-ph2006★ 23 cited

High spatial resolution mid-infrared spectroscopy of the starburst galaxies NGC 3256, IIZw40 and Henize 2-10

N. L. Martin-Hernandez, D. Schaerer, E. Peeters +2

In order to show the importance of high spatial resolution observations of extra-galactic sources when compared to observations obtained with larger apertures such as ISO, we prese…