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- | HOME PAGE | + | ===== 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:\\ | ||
+ | |||
+ | * **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. | ||
+ | |||
+ | ==== 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, theoretical simulations, and astrophysical observations. | ||
+ | * **Tools to model spectra** in astrophysical environments using experimental and theoretical data. | ||