This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
activities [2020/11/10 13:44] cjoblin |
activities [2024/10/28 15:53] (current) cjoblin |
||
---|---|---|---|
Line 1: | Line 1: | ||
- | * 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 **of astrophysical interest**, as well as tools to analyze astronomical data. |
- | - IR spectra obtained with the ESPOIRS setup --> database of Hot PAHs IR spectroscopy | + | More specifically, we cover the following topics: |
+ | |||
+ | ** * 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 | ||
+ | |||
+ | |||
- | * Mass spectrometry | ||
- | * Stability |