Aims.Rates for rotational excitation of ${\rm HC_3N}$ by collisions with He atoms and H2 molecules are computed for kinetic temperatures in the range 5-20 K and 5-100 K, respectively. Methods.These rates are obtained from extensive quantum and quasi-classical calculations using new accurate potential energy surfaces (PES). The ${\rm HC_3N}$–He PES is in excellent agreement with the recent literature. The ${\rm HC_3N}$–H2 angular dependence is approximated using 5 independent H2 orientations. An accurate angular expansion of both PES suitable for low energy scattering is achieved despite the severe steric hindrance effects by the ${\rm HC_3N}$ rod. Results.The rod-like symmetry of the PES strongly favours even $\Delta J$ tra...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
Classical trajectory calculations of the cross sections for vibrational and rotational energy exchan...
Aims.Using a newly determined 5D potential energy surface for H2–H2O we provide an extended and revi...
Aims.Rates for rotational excitation of ${\rm HC_3N}$ by collisions with He atoms and H2 molecules a...
International audienceAims.Rates for rotational excitation of HC_3N by collisions with He atoms and ...
Rates for rotational excitation of HC3N by collisions with He atoms and H2 molecules are computed fo...
Rotational excitation of the interstellar HC2NC and HNC3 molecules, two isomers of HC3N, induced by ...
International audienceModelling of molecular emission from interstellar clouds requires the calculat...
Context. An accurate analysis of the physical-chemical conditions in the regions of the interstellar...
Rate coefficients for rotational transitions in H2 induced by H2 impact are presented. Extensive qua...
This is the published version, also available here: http://dx.doi.org/10.1063/1.430285.The effective...
Rate coefficients for pure rotational quenching in H2(ν 1 = 0, j 1) + H2(ν 2 = 0, j 2) collisions fr...
International audienceThe HCO + and DCO + molecules are commonly used as tracers in the interstellar...
Among the closed-shell hydrocarbons, the carbenes c- and l-C3H2 are the lightest ones to display a p...
9 pags., 8 figs., 1 tab.Accurate modeling of anionic abundances in the interstellar and circumstella...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
Classical trajectory calculations of the cross sections for vibrational and rotational energy exchan...
Aims.Using a newly determined 5D potential energy surface for H2–H2O we provide an extended and revi...
Aims.Rates for rotational excitation of ${\rm HC_3N}$ by collisions with He atoms and H2 molecules a...
International audienceAims.Rates for rotational excitation of HC_3N by collisions with He atoms and ...
Rates for rotational excitation of HC3N by collisions with He atoms and H2 molecules are computed fo...
Rotational excitation of the interstellar HC2NC and HNC3 molecules, two isomers of HC3N, induced by ...
International audienceModelling of molecular emission from interstellar clouds requires the calculat...
Context. An accurate analysis of the physical-chemical conditions in the regions of the interstellar...
Rate coefficients for rotational transitions in H2 induced by H2 impact are presented. Extensive qua...
This is the published version, also available here: http://dx.doi.org/10.1063/1.430285.The effective...
Rate coefficients for pure rotational quenching in H2(ν 1 = 0, j 1) + H2(ν 2 = 0, j 2) collisions fr...
International audienceThe HCO + and DCO + molecules are commonly used as tracers in the interstellar...
Among the closed-shell hydrocarbons, the carbenes c- and l-C3H2 are the lightest ones to display a p...
9 pags., 8 figs., 1 tab.Accurate modeling of anionic abundances in the interstellar and circumstella...
International audienceFrom a new two-dimensional Potential Energy Surface (PES), rotational excitati...
Classical trajectory calculations of the cross sections for vibrational and rotational energy exchan...
Aims.Using a newly determined 5D potential energy surface for H2–H2O we provide an extended and revi...