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Low frequency Carbon Recombination Lines
Published online by Cambridge University Press: 26 May 2016
Abstract
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Low frequency carbon recombination lines with wavelengths up to twenty five meters became important means of low density interstellar plasma diagnostic. Over the past twenty years impressive amount of information was obtained for Cassiopeia A and other galactic directions.
- Type
- Part 6: Spectral Studies of our Galaxy
- Information
- Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 327 - 334
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
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