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Theoretical PAH emission models for aromatic infrared bands
Published online by Cambridge University Press: 01 February 2008
Abstract
Aromatic Infrared Bands (AIBs) show significant profile variations in different astrophysical environments. Theoretical IR data is used to develop emission models to understand these variations. A good match with the observed “7.7” μm feature from different regions is obtained.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S251: Organic Matter in Space , February 2008 , pp. 367 - 368
- Copyright
- Copyright © International Astronomical Union 2008