| Determining gravitational wave radiation from close galaxy pairs using a binary population synthesis approach | |
Liu, J.1 ; Zhang, Y.2,3; Zhang, H.1; Sun, Y.2; Wang, N.1
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| 2012-04-01 | |
| Source Publication | ASTRONOMY & ASTROPHYSICS
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| ISSN | 0004-6361 |
| Volume | 540Pages:A67 |
| Contribution Rank | 1 |
| Abstract | Context. The early phase of the coalescence of supermassive black hole (SMBH) binaries from their host galaxies provides a guaranteed source of low-frequency (nHz-mu Hz) gravitational wave (GW) radiation by pulsar timing observations. These types of GW sources would survive the coalescing and be potentially identifiable. |
| Keyword | Binaries: General Black Hole Physics Stars: Evolution Gravitational Waves |
| Subtype | Article |
| Subject Area | 致密天体、高能和基础物理 |
| DOI | 10.1051/0004-6361/201117501 |
| WOS Headings | Science & Technology ; Physical Sciences |
| URL | 查看原文 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | Black-hole Binaries ; Double White-dwarfs ; Pulsar Timing Arrays ; Digital Sky Survey ; Model ; Mass ; Evolution ; Objects ; Bursts ; Nuclei |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000303315400081 |
| Funding Organization | the program of the light in China's Western Region (LCWR) (No. XBBS201022) ; Natural Science Foundation (No. 11103054) ; Xinjiang Natural Science Foundation (No. 2011211A104) ; John Templeton Foundation(No. 100020101) |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/434 |
| Collection | 其它 射电天文研究室 光学天文与技术应用研究室 计算机技术应用研究室 |
| Corresponding Author | Liu, J. |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Observ, Natl Astron Observ, Xinjiang 830011, Peoples R China 2.Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China 3.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China |
| Recommended Citation GB/T 7714 | Liu, J.,Zhang, Y.,Zhang, H.,et al. Determining gravitational wave radiation from close galaxy pairs using a binary population synthesis approach[J]. ASTRONOMY & ASTROPHYSICS,2012,540:A67. |
| APA | Liu, J.,Zhang, Y.,Zhang, H.,Sun, Y.,&Wang, N..(2012).Determining gravitational wave radiation from close galaxy pairs using a binary population synthesis approach.ASTRONOMY & ASTROPHYSICS,540,A67. |
| MLA | Liu, J.,et al."Determining gravitational wave radiation from close galaxy pairs using a binary population synthesis approach".ASTRONOMY & ASTROPHYSICS 540(2012):A67. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Determining gravitat（576KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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