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Cited article:

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3D structure of H ii regions in the star-forming complex S254-S258

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Dark cloud-type chemistry in photodissociation regions with moderate ultraviolet field

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H-, He-like recombination spectra – III. n-changing collisions in highly excited Rydberg states and their impact on the radio, IR, and optical recombination lines

G J Ferland, N R Badnell, M Dehghanian, et al.
Monthly Notices of the Royal Astronomical Society 486 (1) 1003 (2019)
https://doi.org/10.1093/mnras/stz857

Radio Recombination Lines in Orion A at 8 and 13 mm: The Ionization Structure and Effective Temperature of the Star θ1 C Ori, the Electron Temperature of the Ionized Gas and Turbulence

A. P. Tsivilev, V. V. Krasnov and S. V. Logvinenko
Astronomy Letters 45 (1) 20 (2019)
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Physical parameters of the Orion Bar photodissociation region from radio recombination line observations at 8 mm

A. P. Tsivilev
Astronomy Letters 40 (10) 615 (2014)
https://doi.org/10.1134/S1063773714100077

Determination of the primordial helium abundance from radio recombination line observations: New data. The source W51

A. P. Tsivilev, S. Yu. Parfenov, A. M. Sobolev and V. V. Krasnov
Astronomy Letters 39 (11) 737 (2013)
https://doi.org/10.1134/S106377371310006X