Interstellar PAHs

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PAH Formation and Shocks Cernicharo et al,ApJ, 546, L123 & L127 • The young PNe, GL 618, shows evidence for benzene • Strong shocks, processing a dense toroid of C-rich gas
Benzene Formation in Dense, Warm, Partially Ionized Environments Ion-molecule chemistry driven by an assumed high ionization rate in the presence of acetylene Woods et al, 2002, ApJ, 574, L167
Page 1 and 2: Interstellar PAHs Xander Tielens Le
Page 3 and 4: The incredibly rich spectrum of int
Page 5: PAHs and PDRs in Orion
Page 8 and 9: PAHs as a Measure of Starburst Acti
Page 10 and 11: PAHs and the Universe • PAHs as t
Page 12 and 13: Interstellar PAHs
Page 14 and 15: A day in the life …..
Page 16 and 17: The Relationship of PAHs & Dust PAH
Page 18 and 19: • Wide variety of techniques Spec
Page 20 and 21: Spectral Characteristics II Peeters
Page 22 and 23: • Ratio of C-H/C-C modes measures
Page 24 and 25: Chemical Modification of PAHs • N
Page 26 and 27: Boersma et al, 2008, A & A, 484, 24
Page 28 and 29: Cosmic Journey of Interstellar PAHs
Page 30 and 31: PAH Formation in Stellar Ejecta •
Page 34 and 35: Benzene Formation in Cold Disks Ion
Page 36 and 37: PAH Destruction
Page 38 and 39: Energetic Ion Interaction with PAHs
Page 40 and 41: The ISM is a Harsh Mistress • Lif
Page 42 and 43: IR emission spectra are very simila
Page 44 and 45: SUMMARY • PAHs are everywhere !

Interstellar PAHs

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