Methylacetylene (CH3CCH) and propene (C3H6) formation in cold dense clouds: a case of dust grain chemistry
Langue
en
Article de revue
Ce document a été publié dans
Molecular Astrophysics. 2016-03, vol. 3, p. 1-9
Elsevier
Résumé en anglais
We present an extensive review of gas phase reactions producing methylacetylene and propene showing that these relatively abundant unsaturated hydrocarbons cannot be synthesized through gas-phase reactions. We explain the ...Lire la suite >
We present an extensive review of gas phase reactions producing methylacetylene and propene showing that these relatively abundant unsaturated hydrocarbons cannot be synthesized through gas-phase reactions. We explain the formation of propene and methylacetylene through surface hydrogenation of C3 depleted onto interstellar ices, C3 being a very abundant species in the gas phase.< Réduire
Mots clés en anglais
Physics - Chemical Physics
Astrophysics - Astrophysics of Galaxies
Origine
Importé de halUnités de recherche