Misalignment in the radio jets of NGC 6251

Details Misalignment in the radio jets of NGC 6251 Misalignment in the radio jets of NGC 6251

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...233l.101c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 233, Nov. 1, 1979, p. L101-L104.

Astronomy and Astrophysics

Astronomy

33

Galactic Nuclei, Galactic Structure, Radio Jets (Astronomy), Very Long Base Interferometry, Astronomical Maps, Centimeter Waves, Jets, Optical Thickness, Radio Interferometers

Scientific paper

The compact nuclear source in NGC 6251 has been observed with VLBI
techniques at 2.8 and 13 cm. The source is asymmetric with a bright
optically thick core and an optically thin jet. The jet has a small but
significant difference in position angle from the outer jet.

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