dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade de São Paulo (USP)
dc.date.accessioned2018-11-26T17:51:45Z
dc.date.available2018-11-26T17:51:45Z
dc.date.created2018-11-26T17:51:45Z
dc.date.issued2018-06-01
dc.identifierMonthly Notices Of The Royal Astronomical Society. Oxford: Oxford Univ Press, v. 477, n. 1, p. 548-551, 2018.
dc.identifier0035-8711
dc.identifierhttp://hdl.handle.net/11449/164224
dc.identifier10.1093/mnras/sty753
dc.identifierWOS:000432660300038
dc.identifierWOS000432660300038.pdf
dc.description.abstractThe rate coefficient for the formation of aluminium monochloride, AlCl, from the radiative association of aluminium and chlorine atoms is estimated as a function of temperature. The coupling of the Al and Cl atoms through the A(1)Pi molecular electronic state, which undergoes radiative transition to the X-1 Sigma(+) ground state, is the most efficient transition to form AlCl. The rate constant was found to vary with temperature according to the expressions k(T) = 1.22 x 10(-16)(T/300)(0.40) exp (-748/T) cm(3) s(-1) for temperatures between 300 and 1000 K, and k(T) = 2.20 x 10(-16)(T/300)(0.175)exp (-1067/T) cm(3) s(-1) for temperatures between 1000 and 14 000 K.
dc.languageeng
dc.publisherOxford Univ Press
dc.relationMonthly Notices Of The Royal Astronomical Society
dc.relation2,346
dc.rightsAcesso aberto
dc.sourceWeb of Science
dc.subjectatomic data
dc.subjectatomic processes
dc.subjectcircumstellar matter
dc.subjectISM: molecules
dc.titleFormation of AlCl by radiative association
dc.typeArtículos de revistas


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