What powers the PAH emission in galaxies?

Details What powers the PAH emission in galaxies? What powers the PAH emission in galaxies?

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511..283h&link_type=abstract

Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age, held in Siguenza, Spain 24-27 June, 2002. Edited by

Astronomy and Astrophysics

Astronomy

3

Scientific paper

Our new methodology to study dedicated topics on the ISM is based on the use of the 850 μm continuum as a measure of the full amount of dust, and ISOPHOT-S and ISOCAM observations of the PAH features, which are presumably mixed with the ISM. In this poster we focus on the question: Is the PAH emission in galaxies mainly due to starbursts or due to the interstellar radiation field? For details we refer to the paper by Haas, Klaas & Bianchi (2002). Here we give only a brief outline.

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