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The formation of AlF by radiative association
Author(s) -
C. M. Andreazza,
A. A. de Almeida
Publication year - 2013
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stt2109
Subject(s) - radiative transfer , physics , atomic physics , ground state , molecule , stars , astrophysics , quantum mechanics
The formation of the aluminium monofluoride molecule AlF by radiative association of the Al\udand F atoms is estimated. The radiative association of Al(2P) and F(2P) atoms is found to be\uddominated by the approach along theA1 potential energy curve accompanied by spontaneous\udemission into theX1 \ud+ ground state of the AlF. For temperatures ranging from 300 to 14 000 K,\udthe rate coefficients are found to vary from 1.35×10−17 to 9.31×10−16 cm3 s−1, respectively.\udThese values indicate that only a small amount of AlF molecules can be formed by radiative\udassociation in the inner envelope of carbon-rich stars and other hostile environmentsFAPES

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