The radio source Sagittarius A

Details The radio source Sagittarius A The radio source Sagittarius A

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apl....17...45g&link_type=abstract

Astrophysical Letters, vol. 17, no. 1, 1976, p. 45-47.

Astronomy and Astrophysics

Astronomy

6

Microwave Emission, Radio Sources (Astronomy), Radio Spectra, Supernova Remnants, Astronomical Maps, Background Radiation, Galactic Nuclei, High Resolution, Radio Astronomy

Scientific paper

The high-resolution observations of the radio source Sgr A made between 160 MHz and 5 GHz are compared. The western peak, known as Sgr A West, consists of both thermal and nonthermal discrete components. Sgr A East has a nonthermal origin with the discrete components superimposed on a background component about 3 x 5 arcmin in size. The discrete nonthermal components in Sgr A have a steeper spectrum than the background component and may be parts of a supernova-remnant shell.

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