1997
DOI: 10.1016/s0083-6656(97)00012-3
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EVN-merlin observations of 3C66B

Abstract: We present observations of the FRI radiogalaxy 3C66B during a joint EVN + MER-LIN VLBI session in May 1995. The jet is mapped from the 5 mas scale up to about 3 arcmin. The newly mapped VLBI jet shows essentially two elongated blobs in the direction of the brightest kpc jet (NE). We interpret these two blobs in the light of a new model for VLBI jet making use of the two-fluid concept.

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Cited by 4 publications
(3 citation statements)
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References 9 publications
(5 reference statements)
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“…Weak wiggling patterns can be found, in particular at epoch 2001.20, 2001.48, 2002.14, and 2002.45. These parsec-scale characteristics agree with results in the VLBI images previously obtained at 1.6 GHz and 5.0 GHz (Fraix-Burnet et al 1997;Xu et al 2000;Giovannini et al 2001).…”
Section: Structure Of the Jetsupporting
confidence: 91%
See 1 more Smart Citation
“…Weak wiggling patterns can be found, in particular at epoch 2001.20, 2001.48, 2002.14, and 2002.45. These parsec-scale characteristics agree with results in the VLBI images previously obtained at 1.6 GHz and 5.0 GHz (Fraix-Burnet et al 1997;Xu et al 2000;Giovannini et al 2001).…”
Section: Structure Of the Jetsupporting
confidence: 91%
“…High-resolution imaging using very long baseline interferometry (VLBI) has revealed an asymmetric core-jet structure similar to that observed in radio galaxies (Fraix-Burnet et al 1997;Xu et al 2000;Giovannini et al 2001). Obser-vation at 5.0 GHz reveals the presence of a faint counterjet (Giovannini et al 2001).…”
Section: Introductionmentioning
confidence: 68%
“…Four maps were made ( Fig. 1; Despringre, Fraix-Burnet, & Baudry 1997). The WSRT array provides a map of the whole radiogalaxy with a resolution of 5 arcsec.…”
Section: Observations Of 3c 66bmentioning
confidence: 99%