УГЛОВАЯ СТРУКТУРА КВАЗАРА 3С47 В ДЕКАМЕТРОВОМ ДИАПАЗОНЕ ВОЛН

УГЛОВАЯ СТРУКТУРА КВАЗАРА 3С47 В ДЕКАМЕТРОВОМ ДИАПАЗОНЕ ВОЛН

The quasar 3C47 was observed with the URAN network at decameter wavelengths. A model of its angular structure consisting of four components was fitted. Lobes of the source are enlarged significantly in the range if compare with their high frequency dimensions. The hot spots emission is detected at l...

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Veröffentlicht in:Odessa astronomical publications 2011-12, Vol.24, p.103-105
Hauptverfasser: А. Б. Лозинский, Р. А. Лозинский, О. Л. Ивантишин, Ю. В. Романчев, С. Л. Рашковский, В. А. Шепелев, А. И. Браженко, Р. В. Ващишин, О. А. Литвиненко
Format: Artikel
Sprache:eng
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Zusammenfassung:The quasar 3C47 was observed with the URAN network at decameter wavelengths. A model of its angular structure consisting of four components was fitted. Lobes of the source are enlarged significantly in the range if compare with their high frequency dimensions. The hot spots emission is detected at low frequencies but a radio core is disappeared completely due to its flat spectrum.
ISSN:1810-4215
DOI:10.18524/1810-4215.2011.24.85092