13 years of timing of PSR B1259-63 | |
Wang, N![]() | |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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2004-06-21 | |
卷号 | 351期号:2页码:599-606 |
关键词 | binaries : general pulsars : individual : PSR B1259-63 |
ISSN号 | 0035-8711 |
通讯作者 | na.wang@xao.ac.cn |
英文摘要 | This paper summarizes the results of 13 years of timing observations of a unique binary pulsar, PSR B1259-63, which has a massive B2e star companion. The data span encompasses four complete orbits and includes the periastron passages in 1990, 1994, 1997 and 2000. Changes in dispersion measure occurring around the 1994, 1997 and 2000 periastrons are measured and accounted for in the timing analysis. There is good evidence for a small glitch in the pulsar period in 1997 August, not long after the 1997 periastron, and a significant frequency second derivative indicating timing noise. We find that spin-orbit coupling with secular changes in periastron longitude and projected semimajor axis (x) cannot account for the observed period variations over the whole data set. While fitting the data fairly well, changes in pulsar period parameters at each periastron seem ruled out both by X-ray observations and by the large apparent changes in pulsar frequency derivative. Essentially all of the systematic period variations are accounted for by a model consisting of the 1997 August glitch and step changes in x at each periastron. These changes must be due to changes in the orbit inclination, but we can find no plausible mechanism to account for them. It is possible that timing noise may mask the actual changes in orbital parameters at each periastron, but the good fit to the data of the x step-change model suggests that short-term timing noise is not significant. |
学科主题 | 致密天体、高能和基础物理 |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | PSR B1259-63 ; PERIASTRON PASSAGE ; BINARY-SYSTEMS ; PULSAR ; RADIO ; EMISSION ; EVOLUTION ; RECEIVER ; FORMULA ; STARS |
收录类别 | SCI |
资助信息 | 国家自然科学基金 |
原文出处 | http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966/issues |
语种 | 英语 |
WOS记录号 | WOS:000221976900020 |
公开日期 | 2013-03-06 |
内容类型 | 期刊论文 |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/100] ![]() |
专题 | 脉冲星研究团组 新疆天文台_射电天文研究室 新疆天文台_其它 |
作者单位 | 1.Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia 2.CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia 3.CAS, Natl Astron Observ, Urumqi 830011, Peoples R China |
推荐引用方式 GB/T 7714 | Wang, N,Johnston, S,Manchester, RN. 13 years of timing of PSR B1259-63[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2004,351(2):599-606. |
APA | Wang, N,Johnston, S,&Manchester, RN.(2004).13 years of timing of PSR B1259-63.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,351(2),599-606. |
MLA | Wang, N,et al."13 years of timing of PSR B1259-63".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 351.2(2004):599-606. |
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