The sample of 51 sources between declinations 35 deg and 70 deg with galactic latitude greater than 10 deg and flux density greater than or equal to 1.3 Jy at 5 GHz contains 36 objects that are suitable for study by very long baseline interferometry (VLBI). Observations have been made of seven of these with a VLBI array of four antennas at a frequency of 5 GHz with full hour-angle coverage. The results show a wide variety of morphologies: two sources (0133+476 and 0859+470) are only slightly resolved, one is a double source (0923+392 = 4C 39.25) with a constant separation, three (1807+698 = 3C 371, 1828+487 = 3C 380, and 2200+420 = BL Lac) have an elongated linear structure, and the last (0316+413 = 3C 84) is complex.
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Pearson et al. (1981) studied this question.
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