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VLBI Observations of M87

Published online by Cambridge University Press:  14 August 2015

M. J. Reid
Affiliation:
Harvard-Smithsonian Center for Astrophysics
J.H.M.M. Schmitt
Affiliation:
Harvard-Smithsonian Center for Astrophysics
F. N. Owen
Affiliation:
National Radio Astronomy Observatory
R. S. Booth
Affiliation:
Nuffield Radio Astronomy Laboratories
P. N. Wilkinson
Affiliation:
Nuffield Radio Astronomy Laboratories
D. B. Shaffer
Affiliation:
NASA/GSFC and Phoenix Corp.
K. J. Johnston
Affiliation:
U.S. Naval Research Laboratory
P. E. Hardee
Affiliation:
University of Alabama

Extract

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On 1980 February 20 we conducted an 8-station intercontental VLBI experiment in order to study the nucleus and jet of M87 at 1666.6 MHz in right circular polarization. Our array was sensitive to structures from 0.001 to 0.1 arcsec. We made a hybrid map of the nucleus of M87, and also searched for compact structures within the knots of the jet. The map (Figure 1) shows that the nucleus of M87 contains a one-sided jet. This morphology is similar to that observed in many compact extragalactic sources. The position angle of the nuclear jet is 290.5 (±1) degrees, which precisely matches that of the 20 arcsec jet. No bending of the jet through an angle greater than about 2 degrees is observed. The nucleus also contains a large component (>0.1 arcsec) which is elongated along the same position angle as the jet and has a flux density of roughly 1 Jy. This component is fully resolved by the vast majority of our (u, v) points, and we could not map it with standard techniques.

Type
Research Article
Copyright
Copyright © Reidel 1982