A radio continuum survey of edge-on spiral galaxies at 90 CM

Details A radio continuum survey of edge-on spiral galaxies at 90 CM A radio continuum survey of edge-on spiral galaxies at 90 CM

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..172h&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 172-173 (SEE N93-26706 10-90)

Astronomy and Astrophysics

Astronomy

Continuums, Energy Dissipation, Radio Emission, Sky Surveys (Astronomy), Spiral Galaxies, Halos, Morphology, Spectra, Statistical Analysis, Synchrotrons

Scientific paper

Accurate spectral indices of the radio emission from both the thin disk and thick disk or halo components are critical to understanding the propagation mechanisms of electrons within spiral galaxies. The spectral indices give information of relative importance of diffusion and synchrotron energy loss in the propagation of electrons in the disk. Our goal of this survey is to locate a larger sample of spiral galaxies that exhibit halo phenomena so that a statistical analysis will be possible.

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