Issue |
A&A
Volume 386, Number 3, May II 2002
|
|
---|---|---|
Page(s) | 1129 - 1138 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361:20020268 | |
Published online | 15 May 2002 |
Detection of free radicals in low-temperature gas-grain reactions of astrophysical interest
Ioffe Physico-Technical Institute, 26 Politekhnicheskaya, St. Petersburg 194021, Russia
Corresponding author: R. A. Zhitnikov, zhitnikv.mares@pop.ioffe.rssi.ru
Received:
15
October
2001
Accepted:
20
February
2002
For laboratory detection and investigation of free radicals which
often appear in chemical reactions of astrophysical interest either as
important intermediate or as final products, we pioneered the use of
the electron paramagnetic resonance (EPR) technique, which is very
effective in observing these substances. This has allowed both formyl
(HCO and DCO) and methyl (CH3 and CD3) free radicals to be
detected in a sequence of low-temperature gas-grain reactions of H and
D atom addition in solid CO. The solid samples subjected to the EPR study were obtained by simultaneous independent deposition of CO
molecules and either H or D atoms on the substrate cooled to liquid
helium temperatures. The sequence of the H-atom addition gas-grain
reactions in solid CO is acknowledged to be among the fundamental
processes responsible for the synthesis of organic molecules in
interstellar cloud dust grains. The present observation of the above
free radicals confirms that the solid-state gas-grain sequence of the
reactions is efficient at low temperatures; it also suggests that
there should be considerable concentrations of formyl and methyl
radicals in the ISM. Another study concentrated on the formation of
ethyl free radicals (C2H5) in a low-temperature gas-grain
reaction of H-atom abstraction from a C2H6 molecule by free
H-atom in solid CH4. These experiments were carried out by
deposition onto a substrate, cooled by liquid helium, of a flow of
CH4 molecules containing a small amount of impurities such as
ethane molecules (C2H6), free H-atoms and CH3 radicals formed
in a discharge in a pure gaseous methane. EPR spectra of CH3
radicals, H-atoms, and C2H5 radicals matrix-isolated in solid
CH4 were detected. The relative concentrations of the radicals
were found to depend on the experimental conditions. The abstraction
reaction, C2H6 + H C2H5 + H2, took place
in CH4-ice.
Key words: astrochemistry / molecular processes / methods: laboratory / ISM: dust, extinction / ISM: molecules / ISM: atoms
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.