Institutional Repository of Radio Astronomy Research Laboratory
Detection of proper motion in OQ 208? | |
Stanghellini, C1; Liu, X2![]() | |
2002-05-01 | |
Source Publication | NEW ASTRONOMY REVIEWS
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Volume | 46Issue:2-7Pages:287-289 |
Contribution Rank | 2 |
Abstract | We report on an ongoing project aimed to detect the separation speed of the two hot-spots of the Compact Symmetric Object OQ208. Comparing images at 8.4 GHz taken in 6 epochs between 1994 and 1997 we obtain an estimate of 0.061 +/- 0.024 mas/year for the relative motion between the two outer and compact components of the radio source, and a strong upper limit of 0.13 mas/year. (C) 2002 Elsevier Science B.V. All rights reserved. |
Keyword | Galaxies : Evolution Galaxies : Nuclei Galaxies : Individual (Mkn 668 Radio Continuum : Galaxies Oq 208) |
Subtype | Article |
DOI | 10.1016/s1387-6473(01)00195-6 |
WOS Headings | Science & Technology ; Physical Sciences |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | COMPACT STEEP-SPECTRUM ; RADIO-SOURCES ; YOUNG |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000175717000041 |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/858 |
Collection | 射电天文研究室_星系宇宙学研究团组 射电天文研究室 |
Corresponding Author | Stanghellini, C |
Affiliation | 1.CNR, Ist Radioastron, I-96017 Noto, SR, Italy 2.Chinese Acad Sci, NAO, Urumqi Astron Observ, Urumqi, Peoples R China 3.Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy 4.CNR, Ist Radioastron, I-40129 Bologna, Italy |
Recommended Citation GB/T 7714 | Stanghellini, C,Liu, X,Dallacasa, D,et al. Detection of proper motion in OQ 208?[J]. NEW ASTRONOMY REVIEWS,2002,46(2-7):287-289. |
APA | Stanghellini, C,Liu, X,Dallacasa, D,&Bondi, M.(2002).Detection of proper motion in OQ 208?.NEW ASTRONOMY REVIEWS,46(2-7),287-289. |
MLA | Stanghellini, C,et al."Detection of proper motion in OQ 208?".NEW ASTRONOMY REVIEWS 46.2-7(2002):287-289. |
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Detection of proper (75KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text |
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