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Radio Continuum Emission from Magellanic-Type and Dwarf Irregular Galaxies
Published online by Cambridge University Press: 04 August 2017
Extract
High-frequency radio continuum observations of a small sample of irregular and dwarf galaxies (Klein et al., 1983) have revealed that their integrated radio continuum spectra tend to be significantly flatter than those found for normal spirals (Gioia et al., 1982). This indicates a higher relative amount of thermal (free-free) emission.
- Type
- Supernova Remnants, Radio Continuum, X-ray Sources
- Information
- Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 313 - 314
- Copyright
- Copyright © Reidel 1984