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Дата изменения: Mon Oct 16 15:46:40 2000
Дата индексирования: Mon Oct 1 22:37:24 2012
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Comment on J1239-1023

No image is shown by Dallacasa et al. (1998) as they did not find the VLBI structure at 2.3 and 8.4 GHz prominent, just dominated by a compact region barely resolved in position angle about -45°. In our case the source is well resolved, with a jet pointing to the W-NW direction, in agreement with what is seen in the images at 2.3 and 8.4 GHz from the VLBA Calibrators database.

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Last modified: 16 Oct 2000