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Theoretical PAH emission models for aromatic infrared bands

Published online by Cambridge University Press:  01 February 2008

Amit Pathak  and
Shantanu Rastogi
Amit Pathak
Affiliation:
Physics Department, D. D. U. Gorakhpur University, Gorakhpur - 273009, INDIA. email: [email protected]
Shantanu Rastogi
Affiliation:
Physics Department, D. D. U. Gorakhpur University, Gorakhpur - 273009, INDIA. email: [email protected]
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Abstract

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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.

Keywords

Astrochemistrystars: circumstellar matterinfrared: ISM
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

References

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