The interpretation of hydrogen radio recombination lines
- 1 August 1969
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 4 (4) , 401-416
- https://doi.org/10.1007/bf00651346
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
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- Model Calculations of H II Region TemperaturesPublications of the Astronomical Society of the Pacific, 1967
- Observations of the Hydrogen Recombination Line 158α in Galactic H II RegionsThe Astrophysical Journal, 1967
- On the Determination of the Election Temperatures of H II Regions from the Radio-Frequency Recombination Lines of HydrogenThe Astrophysical Journal, 1967
- Stark Broadening by Electron and Ion Impacts of NA Hydrogen Lines of Large Principal Quantum NumberThe Astrophysical Journal, 1967
- Galactic H II Regions. I. Observations of Their Continuum Radiation at the Frequency 5 GHzThe Astrophysical Journal, 1967
- Galactic H II Regions. II. Observations of Their Hydrogen 109α Recombination-Line Radiation at the Frequency 5009 MHzThe Astrophysical Journal, 1967
- Stimulated Emission of Radio-Frequency Lines of HydrogenThe Astrophysical Journal, 1966
- The Shape of Spectral Lines: Tables of the Voigt ProfileAustralian Journal of Physics, 1959
- Electron Densities in the Orion NEBULA.II.The Astrophysical Journal, 1959