Figure 4 from Low-frequency Carbon Radio Recombination Lines. I. Calculations of Departure Coefficients

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Low-frequency Carbon Radio Recombination Lines. I. Calculations of Departure Coefficients

Authors: F. Salgado, L. K. Morabito, J. B. R. Oonk, P. Salas, M. C. Toribio, H. J. A. Röttgering, and A. G. G. M. Tielens

2017 The Astrophysical Journal 837 141.

Provider: AAS Journals

Caption: Figure 4.

Example of hydrogenic b_nl values at low densities (left panel) and high densities (right panel). A statistical distribution of the l sublevels is attained at levels as low as ∼40. For lower levels, radiative processes dominate the level population. At low density (left panel), radiative processes dominate even at high n levels.

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