The synthesis of complex molecules in interstellar clouds

Citations Over TimeTop 10% of 1979 papers

Abstract

The abundances of polyatomic molecules that may be formed by CH3(+) radiative association reactions in dense interstellar molecular clouds are reevaluated. The formation of a number of complex interstellar molecules via radiative association reactions involving ionic precursors other than CH3(+) is also investigated; these additional precursors include CH3O(+), CH3CO(+), CH5(+), HCO(+), NO(+), H2CN(+), C2H2(+), and NH3(+). The results indicate that the postulated gas-phase ion-molecule radiative association reactions could potentially explain the synthesis of most of the more complex species observed in dense molecular clouds such as Sgr B2. It is concluded, however, that in order to be conclusive, laboratory data are needed to show whether or not these reactions proceed at the required rates at low temperatures.

Related Papers

• → Cosmic-ray astrochemistry(2013)46 cited
• → Astrochemistry(2015)45 cited
• → Anatomy of Orion Molecular Clouds—The Astrochemistry Perspective/Approach(2021)5 cited
• → Reduced networks governing the fractional ionisation in interstellar molecular clouds(2002)12 cited
• → Astrochemistry: Chemistry in dynamically evolving interstellar clouds(1985)