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Emission Lines of [Cl II] in the Optical Spectra of Gaseous Nebulae

  • Authors: F. P. Keenan, L. H. Aller, K. M. Exter, S. Hyung, and D. L. Pollacco

Keenan et al. 2003 The Astrophysical Journal 584 385.

  • Provider: AAS Journals

Caption: Fig. 2.

Theoretical [Cl II] line intensity ratio ﹩R_{1}=I( 3s^{2}3p^{4}﹩ 1D2–﹩3s^{2}3p^{4}﹩ 1S0)﹩/I( 3s^{2}3p^{43}P_{2}﹩–﹩3s^{2}3p^{4}﹩ 1D2) ﹩=I﹩(6161.8 Å)﹩/I﹩(8578.7 Å), where I is in energy units plotted as a function of logarithmic electron density (﹩N_{e}﹩ in cm−3) at an electron temperature of ﹩T_{e}=10^{4.1}﹩ K. Solid line: Calculations with the electron impact excitation rates of Wilson & Bell (2002). Dashed line: Calculations with the atomic data of Krueger & Czyzak (1970).

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