Figure 10 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 10.

Difference between the emissivities (normalized to Hβ) for low nl lines at low density and the results from Martin (1988) in the low-N_e approximation. Our results agree to better than 1% at most levels.

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