Observations of eight supernova remnants at 15 GHz

Details Observations of eight supernova remnants at 15 GHz Observations of eight supernova remnants at 15 GHz

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....44..187g&link_type=abstract

Astronomy and Astrophysics, vol. 44, no. 1, Nov. 1975, p. 187-194.

Astronomy and Astrophysics

Astronomy

17

Astronomical Maps, Brightness Temperature, Polarized Electromagnetic Radiation, Radio Astronomy, Supernova Remnants, Astronomical Models, Radio Telescopes, Tables (Data)

Scientific paper

Eight supernova remnants have been observed with the 100-m radiotelescope at a frequency of 15.0 GHz. The spatial resolution is 58 arcseconds. Maps are presented of Cassiopeia A and Taurus A in both linear polarization and total intensity, and of Tycho's SNR, 3 C 58 and W 49 B in total intensity only. Limits to the brightness temperatures of Kepler's SNR, 3 C 391 and 3 C 397 are also given.

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