148 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR6 papers
- Instituto de Física FundamentalES6 papers
- Institut des Sciences MoléculairesFR3 papers
- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR3 papers
- Université de BordeauxFR3 papers
- Université Le Havre NormandieFR3 papers
- University of Kurdistan HewlerIQ3 papers
- Gyeongsang National UniversityKR2 papers
- Institut de Planétologie et d'Astrophysique de GrenobleFR2 papers
- Laboratoire d'Astrophysique de BordeauxFR2 papers
- Laboratoire Ondes et Milieux ComplexesFR2 papers
- Leiden UniversityNL2 papers
4 papers · 1 filter
Gas phase Elemental abundances in Molecular cloudS (GEMS) VIII. Unlocking the CS chemistry: the CH + S CS + H and C + S CS + C reactions
Carlos M. R. Rocha, Octavio Roncero, Niyazi Bulut +15
We revise the rates of reactions CH + S -> CS + H and C_2 + S -> CS + C, important CS formation routes in dark and diffuse warm gas. We performed ab initio calculations to characte…
Gas-phase Elemental abundances in Molecular cloudS (GEMS) III. Unlocking the CS chemistry: the CS+O reaction
N. Bulut, O. Roncero, A. Aguado +36
CS is among the most abundant gas-phase S-bearing molecules in cold dark molecular clouds. It is easily observable with several transitions in the millimeter wavelength range, and…
Formation of interstellar SH from vibrationally excited H: Quantum study of S + H SH + H reactions and inelastic collisions
Alexandre Zanchet, Francois Lique, Octavio Roncero +2
The rate constants for the formation, destruction, and collisional excitation of SH are calculated from quantum mechanical approaches using two new SH potential energy su…
State-to-state chemistry and rotational excitation of CH in photon-dominated regions
A. Faure, P. Halvick, T. Stoecklin +9
We present a detailed theoretical study of the rotational excitation of CH due to reactive and nonreactive collisions involving C, H, CH, H and free electrons.…