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| + | ===== COSMIC PAH portal ===== | ||
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| + | ==== Description ==== | ||
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| + | Polycyclic aromatic hydrocarbons (PAHs) and related molecular species (e.g. fullerenes) are key species in astrophysical environments. | ||
| + | The primary objective of the Cosmic PAH portal is to ease access to databases and tools | ||
| + | in order to:\\ | ||
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| + | * **Identify** these species in astrophysical environments and in extraterrestrial samples. | ||
| + | * **Understand** their formation pathways and their link with related molecular species such as carbon clusters and fullerenes. | ||
| + | * **Model** their evolution in astrophysical environments and their impact on the physical and chemical conditions. | ||
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| + | ==== Link content ==== | ||
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| + | * **Molecular databases** developed by the team, both theoretical and experimental. | ||
| + | * **Simulated spectra databases** for PAH infrared emission in various astrophysical environments. | ||
| + | * **Spectral analysis tools** to analyze in a consistent way spectra from experiments, | ||
| + | * **Tools to model spectra** in astrophysical environments using experimental and theoretical data. | ||
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