The structure and identification of 3C 105

Details The structure and identification of 3C 105 The structure and identification of 3C 105

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....71..253w&link_type=abstract

Astronomy and Astrophysics, vol. 71, no. 1-2, Jan. 1979, p. 253, 254.

Astronomy and Astrophysics

Astrophysics

Astronomical Maps, Galactic Structure, Magnetic Fields, Radio Galaxies, Astronomical Coordinates, Centimeter Waves, Morphology

Scientific paper

The identification of 3C 105 with an 18.5-mag galaxy proposed as the identification by Smith et al. (1976) is confirmed. The radio structure of this source is very asymmetrical, with about 50% of the 6-cm flux density contained in a compact (angular size less than about 3 arcsec) feature located at the outer edge of the eastern radio lobe. This compact feature is approximately 2.6% polarized at 6 cm; the derived magnetic-field direction is approximately perpendicular to the axis joining the compact feature to the nuclear component.

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