7 pags., 6 figs.Rate coefficients of the complex-forming C + NH→H + CN reaction have been calculated at temperatures ranging from 5 K to 800 K using quasi-classical trajectories on a potential energy surface which accurately describes the attractive long-range interaction, along with results using two capture models. In contrast with the constant value recommended in astrochemical databases, a steep decrease of the rates has been found up to 150 K, and then they tends to be nearly constant. Such behavior is analyzed in terms of the rovibrational state-selected rate coefficients and cross sections singling out the role played by the rotational excitation of the initial diatom. The effect of the electronic degeneracy is also discussed.We than...
International audienceThe reaction between cyano radicals (which are ubiquitous in interstellar clou...
More than 70 molecules of varied nature have been identified in the envelopes of carbon-rich stars t...
The reaction between cyano radicals (which are ubiquitous in interstellar clouds) and methylamine (a...
Rate coefficients for direct radiative association of carbon and nitrogen atoms to form CN, and of c...
International audienceThe investigation of the chemical complexity of hot environments, ranging from...
Among the interstellar molecules, the CN radical is of particular interest since it is a good probe ...
International audienceThe reaction of CN radicals with HC3N is of interest for interstellar and circ...
We carry out quasi-classical trajectory calculations for the C + CH+â C2++ H reaction on an ad hoc c...
[EN] We carry out quasi-classical trajectory caculations for theC + CH+ → C2+ + H reaction on an ad ...
Thermal rate coefficients for the reactions C(3P) + NO(X2Π) → CN(X2Σ+) + O(3P), C(3P) + NO(X2Π) → CO...
Thermal rate coefficients for the reactions C(3P) + NO(X2Π) → CN(X2Σ+) + O(3P), C(3P) + NO(X2Π) → CO...
We carry out quasi-classical trajectory calculations for the C + CH+\ue2\u86\u92 C2++ H reaction on ...
Using a continuous flow CRESU (Cinetique de Reaction en Ecoulement Supersonique Uniforme or Reaction...
The title reaction is thought to be responsible for the production of molecular nitrogen in interste...
International audienceThe investigation of the chemical complexity of hot environments, ranging from...
International audienceThe reaction between cyano radicals (which are ubiquitous in interstellar clou...
More than 70 molecules of varied nature have been identified in the envelopes of carbon-rich stars t...
The reaction between cyano radicals (which are ubiquitous in interstellar clouds) and methylamine (a...
Rate coefficients for direct radiative association of carbon and nitrogen atoms to form CN, and of c...
International audienceThe investigation of the chemical complexity of hot environments, ranging from...
Among the interstellar molecules, the CN radical is of particular interest since it is a good probe ...
International audienceThe reaction of CN radicals with HC3N is of interest for interstellar and circ...
We carry out quasi-classical trajectory calculations for the C + CH+â C2++ H reaction on an ad hoc c...
[EN] We carry out quasi-classical trajectory caculations for theC + CH+ → C2+ + H reaction on an ad ...
Thermal rate coefficients for the reactions C(3P) + NO(X2Π) → CN(X2Σ+) + O(3P), C(3P) + NO(X2Π) → CO...
Thermal rate coefficients for the reactions C(3P) + NO(X2Π) → CN(X2Σ+) + O(3P), C(3P) + NO(X2Π) → CO...
We carry out quasi-classical trajectory calculations for the C + CH+\ue2\u86\u92 C2++ H reaction on ...
Using a continuous flow CRESU (Cinetique de Reaction en Ecoulement Supersonique Uniforme or Reaction...
The title reaction is thought to be responsible for the production of molecular nitrogen in interste...
International audienceThe investigation of the chemical complexity of hot environments, ranging from...
International audienceThe reaction between cyano radicals (which are ubiquitous in interstellar clou...
More than 70 molecules of varied nature have been identified in the envelopes of carbon-rich stars t...
The reaction between cyano radicals (which are ubiquitous in interstellar clouds) and methylamine (a...