Bent beams and the overall size of extragalactic radio sources

Details Bent beams and the overall size of extragalactic radio sources Bent beams and the overall size of extragalactic radio sources

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.276..768r&link_type=abstract

Nature, vol. 276, Dec. 21-28, 1978, p. 768-771

Astronomy and Astrophysics

Astronomy

128

Beams (Radiation), Extragalactic Radio Sources, Quasars, Radio Astronomy, Astrometry, Astronomical Maps, Curvature, Morphology, Radio Transmission, Red Shift, Size Determination

Scientific paper

In a small sample of extragalactic radio sources, curvature is found to be a common feature in bright radio components coincident with quasi-stellar objects. In 3C 273 and 3C 345 the curvature is smooth between the nuclear (less than 0.003 arcsec) and the outer (greater than 1 arcsec) regions. This contrasts sharply with objects having comparatively faint central radio components, which are often well aligned with the extended features.

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