Theoretical Modelling of the Infrared Fluorescence by Interstellar Polycyclic Aromatic Hydrocarbons
1992 ◽
Vol 150
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pp. 137-138
Keyword(s):
We modelled the IR emission of interstellar PAHs. Substantial differences between the IR properties of interstellar and laboratory PAHs are found, possibly resulting from ionization. The various IR features being dominated by distinctly different size PAHs, their observed relative intensities are sensitive indicators of the size distribution. A number of applications of our model related to future ISO and SIRTF IR data are pointed out.
2004 ◽
Vol 38
(9)
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pp. 2557-2567
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2017 ◽
Vol 24
(28)
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pp. 22332-22339
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1997 ◽
Vol 60
(1-4)
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pp. 111-128
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2020 ◽
Vol 19
(2)
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pp. 259-273
2020 ◽
Vol 88
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pp. 370-384
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2004 ◽
Vol 47
(3)
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pp. 223-241
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2012 ◽
Vol 12
(18)
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pp. 8877-8887
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