ISO Spectroscopy of PAH Features

Details ISO Spectroscopy of PAH Features ISO Spectroscopy of PAH Features

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..403p&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Infrared spectra of a large sample of (ultra)compact HII regions (UCHII), Herbig Ae/Be stars, post-AGB stars and PNe are obtained with the ISO-SWS spectrograph on board ISO. These data show a wealth of infrared emission features attributed to Polycyclic Aromatic Hydrocarbons (PAHs). Here we focus on three topics, i.e. the new detection of an emission plateau between 15-20 micron and the 16.4 micron feature, the rich 11-15 micron region with the detection of two new features at 13.6 and 14.2 micron and finally the variation in the 6 to 9 micron PAH spectrum.

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