On the Relative "Transparency" of Gas-phase Coronene Molecules to Low-energy Electrons: Effects on the Interstellar Medium

Details On the Relative "Transparency" of Gas-phase Coronene Molecules to Low-energy Electrons: Effects on the Interstellar Medium On the Relative "Transparency" of Gas-phase Coronene Molecules to Low-energy Electrons: Effects on the Interstellar Medium

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011apj...743..151c&link_type=abstract

The Astrophysical Journal, Volume 743, Issue 2, article id. 151 (2011).

Astronomy and Astrophysics

Astronomy

1

Astrochemistry, Magnetic Fields, Molecular Processes, Opacity, Scattering

Scientific paper

Free, gas-phase polycyclic aromatic hydrocarbons (PAHs) are understood to play an important role in the interstellar medium (ISM), as they are thought to significantly contribute to both diffused and unidentified infrared interstellar bands. They are also considered fundamental blocks of the interstellar dust, whose nature has important implications for a plethora of physical and chemical nanoscopic processes within the ISM. Since free electrons represent a versatile alternative way to transport energy in the interstellar space, in this paper we compute from quantum scattering methods the angular redistributions of free electrons by gas-phase coronene molecules, the latter of which are believed to be one of the most representative PAHs, in order to assess their role in describing the efficiency of electron deflection by this molecule. The associated rates can provide useful information about the coupling mechanism between external radio-frequency fields and complex molecular plasmas containing neutral and ionized PAHs. They can also yield information on the possible presence of such species in the dust phase of the medium.

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