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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 3.

The bn values (left) and ﹩{b}_{n}{\beta }_{n}﹩ values (right) for the hydrogenic approximation at ﹩{T}_{e}={10}^{4}\,\mathrm{and}\,{10}^{2}\,{\rm{K}}﹩ (upper and lower panels, respectively) for different densities (Ne, color scale). The departure coefficients obtained using the nl method show a “bump” at low n levels. The strength and position of the “bump” depend on the physical conditions. As density increases, the l-changing collisions redistribute the electron population more effectively.

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