Linear polarization observations in selected celestial zones - The central region of our Galaxy

Details Linear polarization observations in selected celestial zones - The central region of our Galaxy Linear polarization observations in selected celestial zones - The central region of our Galaxy

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apjs...67..279b&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 67, July 1988, p. 279-282.

Astronomy and Astrophysics

Astronomy

4

Galactic Radiation, Linear Polarization, Milky Way Galaxy, Polarization Characteristics, Galactic Nuclei, Interstellar Magnetic Fields, Radio Sources (Astronomy)

Scientific paper

The Algonquin Radio Observatory and the very large array have been used to obtain the linear polarization integrated over the angular size of a radio galaxy or quasar. All sources are located in a celestial angular zone encompassing the central region of the Galaxy. In addition to the total intensity (Stokes I) flux density, the percentage and position angle of the linear polarization (Stokes Q and U) are obtained for 14 sources at several centimetric wavelengths.

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