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Radio Continuum Emission from Magellanic-Type and Dwarf Irregular Galaxies

Published online by Cambridge University Press:  04 August 2017

Ulrich Klein ,
Roland Gräve  and
Rainer Beck
Ulrich Klein
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG
Roland Gräve
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG
Rainer Beck
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg, FRG

Extract

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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 

References

Gerola, H., Seiden, P.E., Schulman, L.S.: 1980, Astrophys. J. 242, pp. 517–527 Google Scholar
Gioia, I.M., Gregorini, L., Klein, U.: 1982, Astron. Astrophys. 116, pp. 164–174 Google Scholar
Klein, U., Gräve, R., Wielebinski, R.: 1983, Astron. Astrophys. 117, pp. 332–342 Google Scholar