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| - | The primary objective of the Cosmic polycyclic aromatic hydrocarbon (PAH) portal is to gather experimental data | + | The main part of the activities are related to laboratory astrophysics in order to provide molecular data on **polycyclic aromatic hydrocarbons (PAHs)** and related species **of astrophysical interest**, as well as tools to analyze astronomical data. |
| - | in order to: | + | More specifically, we cover the following topics: |
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| + | ** * Spectroscopy** | ||
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| + | - Evolution of infrared spectra with temperature. Simulations of the astronomical Aromatic IR Bands. | ||
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| + | - UV/visible spectroscopy. Link with the interstellar extinction curve. | ||
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| + | ** * Photophysics in isolated environments** | ||
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| + | - UV-VUV photodissociation and photoionization. | ||
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| + | - Competition with radiative cooling. | ||
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| + | - Model of the evolution of PAHs in astrophysical environments. | ||
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| + | ** * Mass spectrometry analysis** | ||
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| + | - Characterization of the molecular content of cosmic dust analogues and meteoritic samples. | ||
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| + | 8-O **//These activities were supported by the Nanocosmos ERC Synergy project (G.A. 610256) and CNES (ID 5830).//** 8-O | ||
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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. | ||