The extended non-thermal radio emission from the Small Magellanic Cloud

Details The extended non-thermal radio emission from the Small Magellanic Cloud The extended non-thermal radio emission from the Small Magellanic Cloud

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..693y&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, April 15, 1991, p. 693-697.

Astronomy and Astrophysics

Astronomy

5

Magellanic Clouds, Nonthermal Radiation, Radio Emission, Astronomical Maps, Interstellar Magnetic Fields, Radio Telescopes

Scientific paper

Radio continuum surveys of the Small Magellanic Cloud (SMC) at 843 MHz have been made using the Parkes 64-m radio telescope. After subtracting nonthermal emission from background sources, identified supernova remnants and thermal emissions scaled from an H-alpha map, the resulting large-scale nonthermal emission is used to estimate the distribution of the magnetic field of the SMC.

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