**Table 6:** Results of modelfit - VLBA images.
Source	Component	Peak	Flux	Size	$\alpha_{1.6}^{22}$
		$\left(\frac{{\rm mJy}}{{\rm beam}}\right)$	(mJy)	(mas)
0222+36	core	61	71	2	$0.05 \pm 0.02$
	N jet	6	16	13
	S jet	3	26	29
	total	-	102
0258+35	core	3.3	7.4	6	$-0.24 \pm 0.02$
	blob	7.5	236	44	$0.54 \pm 0.02$
	total	-	243
0648+27	core	4.3	10	5	$0.47 \pm 0.03$
	jet	1.1	3.4	5
	total	-	12.8
1037+30	core	3.4	3.8	5	$0.14 \pm 0.04$
	hot spot	1.0	40	60	$0.46 \pm 0.02$
	total	-	14
1855+37	N.D.

Note - The spectral index for 0222+36 is computed considering the total flux density detected at 1.6 GHz by the VLBA, which extends over a region smaller than the beam of the VLA at 22 GHz. Spectral index uncertainties are $1\sigma$ values.

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Results
	4 Discussion
	5 Conclusions
	References