2013A&A...549A.103C


Query : 2013A&A...549A.103C

2013A&A...549A.103C - Astronomy and Astrophysics, volume 549A103-103 (2013/1-1)

Electron attachment rates for PAH anions in the ISM and dark molecular clouds: dependence on their chemical properties.

CARELLI F., GRASSI T. and GIANTURCO F.A.

Abstract (from CDS):

The attachment of free electrons to polycondensed aromatic ring molecules (PAHs) is studied for the variety of these molecules with different numbers of condensed rings and over a broad range of electron temperatures, using a multichannel quantum scattering approach. The calculations of the relevant cross sections are used in turn to model the corresponding attachment rates for each of the systems under study, and these rates are parametrized as a function of temperature using a commonly employed expression for two-body processes in the interstellar medium (ISM). The scope of this work is to use first principles to establish the influence of chemical properties on the efficiency of the electron-attachment process for PAHs. Quantum multichannel scattering methods are employed to generate the relevant cross sections, hence the attachment rates, using integral elastic cross sections computed over a broad range of relevant energies, from threshold up to 1000K and linking the attachment to low-energy resonant collisions. The rates obtained for the present molecules are found to markedly vary within the test ensemble of the present work and to be lower than the earlier values used for the entire class of PAHs anions, when modelling their evolutions in ISM environments. The effects of such differences on the evolutions of chemical networks that include both PAH and PAH-species are analysed in some detail and related to previous calculations.

Abstract Copyright: ∼

Journal keyword(s): astrochemistry - ISM: molecules - evolution

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME zet Oph Cloud Cld 16 37 09 -10 34.0           ~ 114 0

Query : 2013A&A...549A.103C

Basic data :
NAME zet Oph Cloud -- Cloud
Other object types:
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Cld (2007AJ)
ICRS coord. (ep=J2000) :
16 37 09.0 -10 34 00 [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
16 34 23.6 -10 28 00 [ ]
Gal coord. (ep=J2000) :
006.2802 +23.5898 [ ]
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Identifiers (2) :
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NAME dze Oph Cloud NAME zet Oph Cloud

References (114 between 1850 and 2026) (Total 114)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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