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Low frequency Carbon Recombination Lines

Published online by Cambridge University Press:  26 May 2016

A. A. Konovalenko
A. A. Konovalenko*
Affiliation:
Institute of Radio Astronomy, National Academy of Sciences of Ukraine, 4 Chervonopraporna St., 61002, Kharkov, Ukraine

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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