Radio continuum of the Small Magellanic Cloud at wavelengths 6 and 3.4 CM

Details Radio continuum of the Small Magellanic Cloud at wavelengths 6 and 3.4 CM Radio continuum of the Small Magellanic Cloud at wavelengths 6 and 3.4 CM

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976aujph..29..329m&link_type=abstract

Australian Journal of Physics, vol. 29, Aug. 1976, p. 329-341.

Astronomy and Astrophysics

Astronomy

37

Continuous Spectra, Magellanic Clouds, Radio Sources (Astronomy), Radio Spectra, Astronomical Maps, Continuous Radiation, Hydrogen Clouds, Ionized Gases, Neutral Particles, Radio Telescopes, Superhigh Frequencies

Scientific paper

The radio continuum at wavelength 6 cm has been surveyed in the direction of the Small Magellanic Cloud with a telescope beam of 4.1 arcmin. Only 27 radio sources have been delineated in this galaxy, and details of their positions, flux densities and spectral indices are given. Some supporting observations were made of the stronger sources at 3.4 cm wavelength. The distribution of the 6 cm emission is compared with the distributions of the ionized gas and neutral hydrogen.

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