activities
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| activities [2021/07/26 11:55] – cjoblin | activities [2026/11/06 16:33] (current) – pah | ||
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| - | ** * Spectroscopy** | + | 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 |
| + | More specifically, | ||
| - | - Evolution of infrared spectra with temperature. | + | * **Spectroscopy** |
| - | - UV/visible spectroscopy. | + | - Evolution of infrared spectra with temperature. Simulations of the astronomical Aromatic IR Bands. |
| - | ** * Photophysics in isolated environments** | + | - UV/visible spectroscopy. Link with the interstellar extinction curve. |
| + | |||
| + | * **Photophysics in isolated environments** | ||
| - UV-VUV photodissociation and photoionization. | - UV-VUV photodissociation and photoionization. | ||
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| - Competition with radiative cooling. | - Competition with radiative cooling. | ||
| - | ** * Mass spectrometry analysis** | + | - Model of the evolution of PAHs in astrophysical environments. |
| + | |||
| + | * **Mass spectrometry analysis** | ||
| - Characterization of the molecular content of cosmic dust analogues and meteoritic samples. | - Characterization of the molecular content of cosmic dust analogues and meteoritic samples. | ||
| + | |||
| + | 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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