Angular structure of extragalactic radio sources at low frequencies

Домашня сторінка
→
Фізико-технічні та математичні науки
→
Відділення фізики і астрономії
→
Кинематика и физика небесных тел
→
Кинематика и физика небесных тел, 2005 (том 21)
→
Кинематика и физика небесных тел, 2005, № 5-додаток
→
Переглянути статтю

Angular structure of extragalactic radio sources at low frequencies

Brazhenko, A.I. ; Koshovy, V.V. ; Lozynsky, A.R. ; Megn, A.V. ; Rashkovsky, S.L. ; Shepelev, V.A.

Тема: MS1: Decameter Radioastronomy

URI: http://dspace.nbuv.gov.ua/handle/123456789/79601

Посилання: Angular structure of extragalactic radio sources at low frequencies / A.I. Brazhenko, V.V. Koshovy, A.R. Lozynsky, A.V. Megn, S.L. Rashkovsky, V.A. Shepelev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 47-50. — Бібліогр.: 2 назв. — англ.

Дата: 2005

Завантажень: 493

Angular structure of extragalactic radio sources at low frequencies

Анотація:

The low frequency VLBI of URAN network operated in the decameter range has been designed in Ukraine to study cosmic radio sources. The network consists of five radio telescopes making up of four interferometers with baselines range from 42 to 913 km with UTR-2 radio telescope operated as the main antenna of the interferometers. The angular resolution of the network amount to 1 arcsec at the highest frequency of the range, and its sensitivity is about 20 Jy. Regular observations of galactic and extragalactic radio sources are performed with the network. Some results of studies are presented here.

Показати повний запис статті