dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.contributor | Universidade de São Paulo (USP) | |
dc.date.accessioned | 2018-11-26T17:51:45Z | |
dc.date.available | 2018-11-26T17:51:45Z | |
dc.date.created | 2018-11-26T17:51:45Z | |
dc.date.issued | 2018-06-01 | |
dc.identifier | Monthly Notices Of The Royal Astronomical Society. Oxford: Oxford Univ Press, v. 477, n. 1, p. 548-551, 2018. | |
dc.identifier | 0035-8711 | |
dc.identifier | http://hdl.handle.net/11449/164224 | |
dc.identifier | 10.1093/mnras/sty753 | |
dc.identifier | WOS:000432660300038 | |
dc.identifier | WOS000432660300038.pdf | |
dc.description.abstract | The 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.language | eng | |
dc.publisher | Oxford Univ Press | |
dc.relation | Monthly Notices Of The Royal Astronomical Society | |
dc.relation | 2,346 | |
dc.rights | Acesso aberto | |
dc.source | Web of Science | |
dc.subject | atomic data | |
dc.subject | atomic processes | |
dc.subject | circumstellar matter | |
dc.subject | ISM: molecules | |
dc.title | Formation of AlCl by radiative association | |
dc.type | Artículos de revistas | |