Multiline observations of hydrogen, helium, and carbon radio-recombination lines toward Orion A: A detailed dynamical study and direct determination of physical conditions

Open Access

Fig. 13

Observed CRRL, [¹²C II], and [¹³C II] intensities constrain electron temperature T_e and electron density n_e (orange, C55α; green, [¹²C II]; blue, [¹³C II]). The shaded area gives the 1σ error of each observation. Each panel uses the respective model grid with the column density inferred from the Bayesian analysis.

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