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The interpretation of hydrogen radio recombination lines

โœ Scribed by J. E. Dyson

Publisher
Springer Netherlands
Year
1969
Tongue
English
Weight
643 KB
Volume
4
Category
Article
ISSN
0004-640X

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๐Ÿ“œ SIMILAR VOLUMES

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Radio recombination lines (RRL.) discovered about 25 years ago became a very effective tool for the investigation of interstellar matter (ISM). These lines are unique by the number of transitions and the spectral range observed: from 2 mm to 20 m wavelength. This allows to study the ISM under variet

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## Litle of program: GENERAL BN PROGRAM Nature of physical problem Emission lines produced by the recombination ofhydrogen Catalogue number: ACXI and hydrogenic ions are observed from many astronomical sources; maser amplification is frequently present. The re-Program obtainable from: CPC Program