9 pags., 8 figs.We present a detailed theoretical study of the rotational excitation of CH+ due to reactive and non-reactive collisions involving C+(2P), H2, CH+, H and free electrons. Specifically, the formation of CH+ proceeds through the reaction between C+(2P) and H2(νH2=1,2), while the collisional (de)excitation and destruction of CH+ is due to collisions with hydrogen atoms and free electrons. State-to-state and initial-state-specific rate coefficients are computed in the kinetic temperature range 10–3000 K for the inelastic, exchange, abstraction and dissociative recombination processes using accurate potential energy surfaces and the best scattering methods. Good agreement, within a factor of 2, is found between the experimental an...
The CH$^+$ ion was one of the first molecules identified in the interstellar gas over 75 years ago, ...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
We present a detailed theoretical study of the rotational excitation of CH+ due to reactive and non...
Aims. Excitation of far-infrared and submillimetric molecular lines may originate from non...
Aims. Excitation of far-infrared and submillimetric molecular lines may originate from non...
Aims. Excitation of far-infrared and submillimetric molecular lines may originate from non...
The CH^+ ion is a key species in the initial steps of interstellar carbon chemistry. Its formation i...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
ABSTRACT Context. The abundances of interstellar CH + and SH + are not well understood as their most...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
The CH$^+$ ion was one of the first molecules identified in the interstellar gas over 75 years ago, ...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
We present a detailed theoretical study of the rotational excitation of CH+ due to reactive and non...
Aims. Excitation of far-infrared and submillimetric molecular lines may originate from non...
Aims. Excitation of far-infrared and submillimetric molecular lines may originate from non...
Aims. Excitation of far-infrared and submillimetric molecular lines may originate from non...
The CH^+ ion is a key species in the initial steps of interstellar carbon chemistry. Its formation i...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
ABSTRACT Context. The abundances of interstellar CH + and SH + are not well understood as their most...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
The CH$^+$ ion was one of the first molecules identified in the interstellar gas over 75 years ago, ...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...
Context. The abundances of interstellar CH+ and SH+ are not well understood as their most likely for...