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| Polycyclic aromatic hydrocarbons (PAHs) and related molecular species (e.g. fullerenes) are key species in astrophysical environments. | 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 molecular data | + | The primary objective of the Cosmic PAH portal is to ease access to databases and tools |
| - | in order to: | + | 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. | + | * **Identify** these species in astrophysical environments and in extraterrestrial samples. |
| - | * Model their evolution in astrophysical environments and their impact on the physical and chemical conditions. | + | * **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 ==== | ==== Link content ==== | ||
| - | * Molecular databases developed by the team, both theoretical and experimental. | + | |
| - | * Databases of modeled spectra in astrophysical environments. | + | * **Molecular databases** developed by the team, both theoretical and experimental. |
| - | * Tools to analyze in a consistent way spectra from experiments. theoretical calculations, and astrophysical observations. | + | * **Simulated spectra databases** for PAH infrared emission in various astrophysical environments. |
| - | * Tools to model spectra in astrophysical environments using experimental and theoretical data. | + | * **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. | ||
home.1642176094.txt.gz · Last modified: 2022/01/14 16:01 by cjoblin
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