Rate coefficients for direct radiative association of carbon and nitrogen atoms to form CN, and of carbon ions and nitrogen atoms to form CN+ ions, are calculated for temperatures in the range of 300 to 14,700 K. For the CN molecule, the rate coefficients can be represented by the standard expression, k(CN)(T) = 7.87 x 10(-19)(T/300)(0.056) exp (-96.0/T) cm(3) s(-1) for temperatures between 300 and 2700 K and k(CN)(T) = 1.37 x 10(-18)(T/300)-0.128 exp (-520.1/T) cm(-3) s(-1) at T > 2700 K. For the CN+ ion, the corresponding expression is k(CN+)(T) = 1.08 x 10(-18)(T/300)(0.071) exp (-57.5/T) cm(-3) s(-1) for the temperature range studied. Calculated rate coefficients k(CN) are about 2 orders of magnitude lower than the canonical value used ...
[EN] We carry out quasi-classical trajectory caculations for theC + CH+ → C2+ + H reaction on an ad ...
This paper deals with the possible formation of two molecular anions often considered like...
We carry out quasi-classical trajectory calculations for the C + CH+\ue2\u86\u92 C2++ H reaction on ...
7 pags., 6 figs.Rate coefficients of the complex-forming C + NH→H + CN reaction have been calculated...
International audienceThe reaction of CN radicals with HC3N is of interest for interstellar and circ...
This thesis is devoted to the theoretical investigation of radiative association, which is one of th...
Among the interstellar molecules, the CN radical is of particular interest since it is a good probe ...
International audienceThe interstellar detection of CH3CN metastable isomers would suggest that CH3N...
International audienceThe reaction between cyano radicals (which are ubiquitous in interstellar clou...
A first-principle theoretical approach to study the process of radiative electron attachment is deve...
International audienceThe reaction between cyano radicals (which are ubiquitous in interstellar clou...
We have investigated the chemistry of C + H3+ forming CH+, CH2+, and CH3+. These reactions are belie...
The reaction between cyano radicals (which are ubiquitous in interstellar clouds) and methylamine (a...
International audienceThe kinetics of the reactions of cyano radical, CN (X2sigma+) with three hydro...
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 ...
This paper deals with the possible formation of two molecular anions often considered like...
We carry out quasi-classical trajectory calculations for the C + CH+\ue2\u86\u92 C2++ H reaction on ...
7 pags., 6 figs.Rate coefficients of the complex-forming C + NH→H + CN reaction have been calculated...
International audienceThe reaction of CN radicals with HC3N is of interest for interstellar and circ...
This thesis is devoted to the theoretical investigation of radiative association, which is one of th...
Among the interstellar molecules, the CN radical is of particular interest since it is a good probe ...
International audienceThe interstellar detection of CH3CN metastable isomers would suggest that CH3N...
International audienceThe reaction between cyano radicals (which are ubiquitous in interstellar clou...
A first-principle theoretical approach to study the process of radiative electron attachment is deve...
International audienceThe reaction between cyano radicals (which are ubiquitous in interstellar clou...
We have investigated the chemistry of C + H3+ forming CH+, CH2+, and CH3+. These reactions are belie...
The reaction between cyano radicals (which are ubiquitous in interstellar clouds) and methylamine (a...
International audienceThe kinetics of the reactions of cyano radical, CN (X2sigma+) with three hydro...
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 ...
This paper deals with the possible formation of two molecular anions often considered like...
We carry out quasi-classical trajectory calculations for the C + CH+\ue2\u86\u92 C2++ H reaction on ...