Theoretical PAH emission models for aromatic infrared bands

Details Theoretical PAH emission models for aromatic infrared bands Theoretical PAH emission models for aromatic infrared bands

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..251..367p&link_type=abstract

Organic Matter in Space, Proceedings of the International Astronomical Union, IAU Symposium, Volume 251, p. 367-368

Astronomy and Astrophysics

Astrophysics

Astrochemistry, Stars: Circumstellar Matter, Infrared: Ism

Scientific paper

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.

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