Jetlike radiostructure in the core of 3C236

Details Jetlike radiostructure in the core of 3C236 Jetlike radiostructure in the core of 3C236

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981esasp.162..107s&link_type=abstract

In ESA Opt. Jets in Galaxies p 107-108 (SEE N81-27993 18-88)

Computer Science

6

Extragalactic Radio Sources, Jets, Radio Emission, Morphology, Radio Galaxies, Radio Spectra, Very Long Base Interferometry

Scientific paper

The fine structure of the core was studied using very long baseline interferometry observations at 18 cm using Effelsberg, Dwingeloo and Jodrell Bank together with a transatlantic baseline to Green Bank. A preliminary hybrid map is shown with a restoring beam appropriate to the European baselines. Although the calibration of the data are not yet complete, the following preliminary conclusions can be drawn: (1) the steep spectrum core of 3C 236 resembles the jet-like structures seen in many sources on a much larger scale; (2) Although the overall extension of the core agrees with that of the outer lobes the existence of non-linear fine structure in the core is confirmed; (3) The bending observed in the south eastern region of the jet resembles the wiggles often seen in larger jets; and (4) There is a gradual change in position angle by 25 deg. From the eastern to the western regions of the core.

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