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Дата изменения: Mon Oct 16 16:08:13 2000
Дата индексирования: Mon Oct 1 22:42:41 2012
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Поисковые слова: наблюдения метеорных потоков
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Comment on J1720-0058

Resolved: this FR-II radio galaxy is not detected at 2.3 GHz by Preston et al. (1985). A VLA map at 8.4 GHz is published by Swain, Bridle & Baum (1998). However, there is correlated signal at the shortest baselines from which a position has been derived and is listed in the table. Our best guess is that the residual core has a flux density of 0.15 Jy and a size of ~15 mas. See Figure 3.

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Last modified: 16 Oct 2000