K. M. Aggarwal
Articles written in Journal of Astrophysics and Astronomy
Volume 9 Issue 4 December 1988 pp 237-241
Volume 10 Issue 2 June 1989 pp 147-150
Relative level populations for O III, derived using electron impact excitation rates calculated with the R-matrix code, are used to deduce the electron-temperature-sensitive emission-line ratio
Volume 40 | Issue 2
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