Electron-impact rotational excitation of the carbon monosulphide (CS) molecule


Autoria(s): Varambhia, H.N.; Faure, A.; Graupner, Karola; Field, Thomas; Tennyson, J.
Data(s)

11/04/2010

Resumo

Rotational excitation of the carbon monosulphide (CS) molecule by thermal electron-impact is studied using the molecular R-matrix method combined with the adiabatic-nuclei-rotation (ANR) approximation. Rate coefficients are obtained for electron temperatures in the range 5-5000 K and for transitions involving levels up to J = 40. It is confirmed that dipole allowed transitions (Delta J = 1) are dominant and that the corresponding rate coefficients exceed those for excitation by neutrals by at least five orders of magnitude. As a result, the present rates should be included in any detailed population model of CS in sources where the electron fraction is larger than similar to 10(-5), in particular in diffuse molecular clouds and interstellar shocks.

Formato

application/pdf

Identificador

http://pure.qub.ac.uk/portal/en/publications/electronimpact-rotational-excitation-of-the-carbon-monosulphide-cs-molecule(2574c38d-549d-417e-a23a-05b0a3ce4921).html

http://dx.doi.org/10.1111/j.1365-2966.2010.16207.x

http://pure.qub.ac.uk/ws/files/776365/2010_CS_MNRAS_roational_excitation.pdf

Idioma(s)

eng

Direitos

info:eu-repo/semantics/restrictedAccess

Fonte

Varambhia , H N , Faure , A , Graupner , K , Field , T & Tennyson , J 2010 , ' Electron-impact rotational excitation of the carbon monosulphide (CS) molecule ' Monthly Notices of the Royal Astronomical Society , vol 403 , no. 3 , pp. 1409-1412 . DOI: 10.1111/j.1365-2966.2010.16207.x

Palavras-Chave #/dk/atira/pure/subjectarea/asjc/1900/1912 #Space and Planetary Science #/dk/atira/pure/subjectarea/asjc/3100/3103 #Astronomy and Astrophysics
Tipo

article