|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2017A&A...598A..22B - Astronomy and Astrophysics, volume 598A, 22-22 (2017/2-1)
CN radical hydrogenation from solid H2 reactions, an alternative way of HCN formation in the interstellar medium.
BORGET F., MULLER S., GROTE D., THEULE P., VINOGRADOFF V., CHIAVASSA T. and SANDER W.
Abstract (from CDS):
Context. Molecular hydrogen (H2) is the most abundant molecule of the interstellar medium (ISM) in gas phase and it has been assumed to exist in solid state or as coating on grains.
Aims. Our goal is to show that solid H2 can act as a hydrogenation agent, reacting with CN radicals to form HCN.
Methods. In a H2 matrix, we studied the hydrogenation of the CN radical generated from the vacuum ultraviolet photolysis (VUV-photolysis) of C2N2 at 3.8K. We modified the wavelengths and the host gas in order to be sure that CN radicals can abstract H from H2 molecules.
Results. HCN monomers, dimers, and oligomers have been characterised by Fourier transform infrared spectroscopy (FTIR). H2CN as well as CN radicals have also been clearly observed during the photolysis performed at 3.8K.
Conclusions. H2 is a hydrogenation reagent towards CN radicals producing HCN. This type of reaction should be taken into account for the reactivity at low temperature in contaminated H2 ice macro-particles (CHIMPs), H2 flakes or in the first sublayers of grains where solid H2 has accumulated.
Aims. Our goal is to show that solid H2 can act as a hydrogenation agent, reacting with CN radicals to form HCN.
Methods. In a H2 matrix, we studied the hydrogenation of the CN radical generated from the vacuum ultraviolet photolysis (VUV-photolysis) of C2N2 at 3.8K. We modified the wavelengths and the host gas in order to be sure that CN radicals can abstract H from H2 molecules.
Results. HCN monomers, dimers, and oligomers have been characterised by Fourier transform infrared spectroscopy (FTIR). H2CN as well as CN radicals have also been clearly observed during the photolysis performed at 3.8K.
Conclusions. H2 is a hydrogenation reagent towards CN radicals producing HCN. This type of reaction should be taken into account for the reactivity at low temperature in contaminated H2 ice macro-particles (CHIMPs), H2 flakes or in the first sublayers of grains where solid H2 has accumulated.
Abstract Copyright: © ESO, 2017
Journal keyword(s): astrochemistry - molecular processes - astrobiology - ISM: molecules
Simbad objects: 1
To bookmark this query, right click on this link: simbad:2017A&A...598A..22B and select 'bookmark this link' or equivalent in the popup menu