Editorial
Foreword
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- 30 March 2011, pp. III-VI
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Research Article
25 years of PAH hypothesis
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- 30 March 2011, pp. 3-10
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Astronomical observations of the PAH emission bands
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- 30 March 2011, pp. 13-27
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Astronomical Models of PAHs and Dust
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- 30 March 2011, pp. 29-42
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Dialectics of the PAH Abundance Trend with Metallicity
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- 30 March 2011, pp. 43-48
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The shape of Mid-IR PAH bands in the Universe
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- 30 March 2011, pp. 49-54
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AKARI Near-Infrared Spectroscopy of 3 micron PAH and 4 micron PAD features
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- 30 March 2011, pp. 55-60
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Laboratory infrared spectroscopy of PAHs
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- 30 March 2011, pp. 61-73
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Computational IR Spectroscopy for PAHs: from the early years to the present status
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- 30 March 2011, pp. 75-93
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Modeling the anharmonic infrared Emission Spectra of PAHs: Application to the Pyrene Cation
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- 30 March 2011, pp. 95-101
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Laboratory Spectroscopy of Protonated PAH Molecules Relevant For Interstellar Chemistry
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- 30 March 2011, pp. 103-108
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The NASA Ames PAH IR Spectroscopic Database and the far-IR
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- 30 March 2011, pp. 109-115
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Analyzing astronomical observations with the NASA Ames PAH database
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- 30 March 2011, pp. 117-122
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Search for far-IR PAH bands with Herschel: modelling and observational approaches
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- 30 March 2011, pp. 123-130
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Polycyclic Aromatic Hydrocarbons as Star Formation Rate Indicators
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- 30 March 2011, pp. 133-141
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PAHs and the ISM in Metal-Poor Starbursts
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- 30 March 2011, pp. 143-148
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Introduction to AMUSES: AKARI survey with a window of opportunity
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- 30 March 2011, pp. 149-154
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PAH evolution in the harsh environment of the ISM
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- 30 March 2011, pp. 157-168
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PAH and Dust Processing in Supernova Remnants
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- 30 March 2011, pp. 169-175
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The formation of Polycyclic Aromatic Hydrocarbons in evolved circumstellar environments
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- 30 March 2011, pp. 177-189
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