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

dc.contributor.author	Brazhenko, A.I.
dc.contributor.author	Koshovy, V.V.
dc.contributor.author	Lozynsky, A.R.
dc.contributor.author	Megn, A.V.
dc.contributor.author	Rashkovsky, S.L.
dc.contributor.author	Shepelev, V.A.
dc.date.accessioned	2015-04-03T15:01:46Z
dc.date.available	2015-04-03T15:01:46Z
dc.date.issued	2005
dc.identifier.citation	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.	uk_UA
dc.identifier.issn	0233-7665
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/79601
dc.description.abstract	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.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Кинематика и физика небесных тел
dc.subject	MS1: Decameter Radioastronomy	uk_UA
dc.title	Angular structure of extragalactic radio sources at low frequencies	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA