Issue |
A&A
Volume 522, November 2010
|
|
---|---|---|
Article Number | A90 | |
Number of page(s) | 8 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361/201014774 | |
Published online | 05 November 2010 |
Experimental studies of the dissociative recombination of
CD3CDOD+ and
CH3CH2OH
1
Department of PhysicsStockholm University,
106 91
Stockholm,
Sweden
e-mail: mh@physto.se
2
Radboud University Nijmegen, Institute for Molecules and
Materials, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
3
Institute of Physics, Jan Kochanowski University,
Świȩtokrzyska 15,
25406
Kielce,
Poland
4
Institute of Modern Physics, Chinese Academy of Sciences, 509 Nanchang Rd.,
Lanzhou
730000, PR
China
5 Department of Physics, Albert-Ludwigs Universität Freiburg,
Hermann-Herder-Str. 3, 79104 Freiburg Germany
6
Manne Siegbahn Laboratory, Frescativägen 26, 114 18
Stockholm,
Sweden
Received:
12
April
2010
Accepted:
22
July
2010
Aims. We determine branching fractions, cross sections and thermal rate
constants for the dissociative recombination of CD3CDOD+ and
CH3CH2OH at the low
relative kinetic energies encountered in the interstellar medium.
Methods. The experiments were carried out by merging an ion and electron beam at the heavy ion storage ring CRYRING, Stockholm, Sweden.
Results. Break-up of the CCO structure into three heavy fragments is not
found for either of the ions. Instead the CCO structure is retained in 23 ± 3% of the DR
reactions of CD3CDOD+ and 7 ± 3% in the DR of
CH3CH2OH, whereas rupture
into two heavy fragments occurs in 77 ± 3% and 93 ± 3% of the DR events of the
respective ions. The measured cross sections were fitted between 1–200 meV yielding the
following thermal rate constants and cross-section dependencies on the relative kinetic
energy:
σ(Ecm [eV] ) = 1.7 ± 0.3 × 10-15(Ecm [eV] ) − 1.23 ± 0.02 cm2
and
k(T) = 1.9 ± 0.4 × 10-6(T / 300) − 0.73 ± 0.02 cm3 s-1
for CH3CH2OH
as well as
k(T) = 1.1 ± 0.4 × 10-6(T / 300) − 0.74 ± 0.05 cm3 s-1
and
σ(Ecm [eV]) = 9.2 ± 4 × 10-16(Ecm [eV] ) − 1.24 ± 0.05 cm2
for CD3CDOD+
Key words: astrochemistry / molecular processes / plasmas / methods: laboratory
© ESO, 2010
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