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Astron. Astrophys. 338, 840-842 (1998)

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5. Conclusion

The observed complex structure and the lack of a well defined radio core in 3C287 indicate that simple precession models cannot describe the source. Both short baselines and quasi-simultaneous multi-frequency observations are needed in order to map the faint surface brightness emission and locate a possible radio core at higher frequencies. These further observations would help us to get a better understanding of the nature of 3C287.

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© European Southern Observatory (ESO) 1998

Online publication: September 17, 1998
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