activities
Differences
This shows you the differences between two versions of the page.
| Both sides previous revisionPrevious revisionNext revision | Previous revision | ||
| activities [2021/07/26 13:26] – cjoblin | activities [2026/11/06 16:33] (current) – pah | ||
|---|---|---|---|
| Line 1: | Line 1: | ||
| - | Scientific | + | 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. |
| + | More specifically, | ||
| - | ** * Spectroscopy** | + | * **Spectroscopy** |
| - Evolution of infrared spectra with temperature. Simulations of the astronomical Aromatic IR Bands. | - Evolution of infrared spectra with temperature. Simulations of the astronomical Aromatic IR Bands. | ||
| Line 7: | Line 8: | ||
| - UV/visible spectroscopy. Link with the interstellar extinction curve. | - UV/visible spectroscopy. Link with the interstellar extinction curve. | ||
| - | ** * Photophysics in isolated environments** | + | * **Photophysics in isolated environments** |
| - UV-VUV photodissociation and photoionization. | - UV-VUV photodissociation and photoionization. | ||
| Line 15: | Line 16: | ||
| - Model of the evolution of PAHs in astrophysical environments. | - Model of the evolution of PAHs in astrophysical environments. | ||
| - | ** * Mass spectrometry analysis** | + | * **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 | ||
activities.1627306013.txt.gz · Last modified: (external edit)
