Oomens
- astrophysical observations
- UIR bands
- possible carriers,
why PAHs?
- emission process
- PAH characteristics
- UV
absorption
- UV photostability and ionization
- neutral vs ionic PAHs
- laboratory spectroscopic
methods
- neutral
- cation
- computational
- spectra of neutrals
- matrix isolation data
- Far
IR spectra
- cation
spectra
- matrix isolation
- comparison between
experimental methods
- matrix isolation vs. gas-phase
- IRMPD
vs linear absorption spectroscopy
- relevance to emission spectra
- Related species
- Fe+PAHs
- N-substituted
PAHs
-
(de)hydrogenated PAHs
- diamondoids
- neutrals
- ions
- Matching the lab spectra with UIR bands
- spectral trends
-
average PAH spectra
- size and charge state of interstellar PAHs
- toward giant PAHs
- Open issues