2009ApJ...695..317V


Query : 2009ApJ...695..317V

2009ApJ...695..317V - Astrophys. J., 695, 317-324 (2009/April-2)

The dissociative recombination of protonated acrylonitrile, CH2CHCNH+, with implications for the nitrile chemistry in dark molecular clouds and the upper atmosphere of Titan.

VIGREN E., HAMBERG M., ZHAUNERCHYK V., KAMINSKA M., THOMAS R.D., LARSSON M., MILLAR T.J., WALSH C. and GEPPERT W.D.

Abstract (from CDS):

Measurements on the dissociative recombination (DR) of protonated acrylonitrile, CH2CHCNH+, have been performed at the heavy ion storage ring CRYRING located in the Manne Siegbahn Laboratory in Stockholm, Sweden. It has been found that at ∼2 meV relative kinetic energy about 50% of the DR events involve only ruptures of X-H bonds (where X = C or N) while the rest leads to the production of a pair of fragments each containing two heavy atoms (alongside H and/or H2). The absolute DR cross section has been investigated for relative kinetic energies ranging from ∼1 meV to 1 eV. The thermal rate coefficient has been determined to follow the expression k(T) = 1.78x10–6 (T/300) – 0.80 cm3/s for electron temperatures ranging from ∼10 to 1000 K. Gas-phase models of the nitrile chemistry in the dark molecular cloud TMC-1 have been run and results are compared with observations. Also, implications of the present results for the nitrile chemistry of Titan's upper atmosphere are discussed.

Abstract Copyright: ∼

Journal keyword(s): ISM: clouds - ISM: molecules - methods: laboratory - molecular processes

Errata: erratum vol. 724, p. 1571 (2010)

Simbad objects: 4

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Number of rows : 4
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 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
2 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1227 1
3 IRC +10216 C* 09 47 57.40632 +13 16 43.5648           C9,5e 2455 0
4 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2443 1

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