Radio Recombination Lines: A New Observational Tool in Astrophysics
- 5 April 1968
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 160 (3823) , 29-42
- https://doi.org/10.1126/science.160.3823.29
Abstract
No abstract availableThis publication has 30 references indexed in Scilit:
- Galactic H II Regions. III. The Nature of the Radio Source W49The 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
- Determination of Election Temperatures from Observations of Radio LinesThe Astrophysical Journal, 1967
- Radio Observations of Interstellar Hydroxyl RadicalsScience, 1967
- Detection of a New Microwave Spectral LineNature, 1967
- High-Resolution Radio Observations of an Intense H II Region in Cygnus XThe Astrophysical Journal, 1967
- Hydrogen Recombination Lines 126α and 166α observed in Galactic HII RegionsNature, 1967
- Detection of Hydrogen Emission Line 166α in M17Nature, 1966
- Temperature in H II Regions and Planetary Nebulae.The Astrophysical Journal, 1965
- OH Emission in the Direction of Radio Source W49Nature, 1965