Methylacetylene (CH3CCH) and propene (C3H6) formation in cold dense clouds: a case of dust grain chemistry
Idioma
en
Article de revue
Este ítem está publicado en
Molecular Astrophysics. 2016-03, vol. 3, p. 1-9
Elsevier
Resumen en inglés
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 ...Leer más >
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.< Leer menos
Palabras clave en inglés
Physics - Chemical Physics
Astrophysics - Astrophysics of Galaxies
Orígen
Importado de HalCentros de investigación