Synchrotron Emission from the Galaxy and the Diffuse X-ray Background

Details Synchrotron Emission from the Galaxy and the Diffuse X-ray Background Synchrotron Emission from the Galaxy and the Diffuse X-ray Background

Dec 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.224.1090h&link_type=abstract

Nature, Volume 224, Issue 5224, pp. 1090-1093 (1969).

Computer Science

5

Scientific paper

MEASUREMENTS of the low-resolution, low-frequency, radio spectra in the direction of the galactic poles show a significant difference between the two hemispheres. Spectra for the north and south galactic poles are shown in Fig. 1, based on refs. 1-19, and the vertical scales have been displaced to assist comparison. The brightness S as a function of frequency ν between 10 and 150 MHz is well described by where the spectral index α has the values α ~= 0.4 for the north galactic halo, and α ~= 0.6 for the south galactic halo.

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