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 10:51] – created cjoblin | activities [2026/11/06 16:33] (current) – pah | ||
|---|---|---|---|
| Line 1: | Line 1: | ||
| - | The primary objective | + | The main part of the activities are related to laboratory astrophysics in order to provide molecular data on **polycyclic aromatic |
| - | in order to: | + | More specifically, |
| + | |||
| + | * **Spectroscopy** | ||
| + | |||
| + | - Evolution of infrared spectra with temperature. Simulations of the astronomical Aromatic IR Bands. | ||
| + | |||
| + | - UV/visible spectroscopy. Link with the interstellar extinction curve. | ||
| + | |||
| + | * **Photophysics in isolated environments** | ||
| + | |||
| + | - UV-VUV photodissociation and photoionization. | ||
| + | |||
| + | - Competition with radiative cooling. | ||
| + | |||
| + | - Model of the evolution of PAHs in astrophysical environments. | ||
| + | |||
| + | * **Mass spectrometry analysis** | ||
| + | |||
| + | - 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 | ||
| + | |||
| - | - 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. | ||
activities.1627296672.txt.gz · Last modified: (external edit)
