Formation of AlCl by radiative association

被引:10
作者
Andreazza, C. M. [1 ]
de Almeida, A. A. [2 ]
Vichietti, R. M. [3 ]
机构
[1] Univ Estadual Paulista, IGCE, DEMAC, Av 24A,1515, BR-13506700 Rio Claro, SP, Brazil
[2] Univ Sao Paulo, IAG, Rua Matao 1226, BR-05508090 Sao Paulo, SP, Brazil
[3] Univ Sao Paulo, IQSC, Av Trabalhador Sao Carlense 400, BR-13566590 Sao Carlos, SP, Brazil
基金
巴西圣保罗研究基金会;
关键词
atomic data; atomic processes; circumstellar matter; ISM: molecules; ASYMPTOTIC GIANT BRANCH; VY-CANIS MAJORIS; EVOLUTION; ALF; IRC+10216; TRANSITION; COLLISIONS; MOLECULES; CHEMISTRY; STARS;
D O I
10.1093/mnras/sty753
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:548 / 551
页数:4
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