Ultraluminous X-ray pulsar: Accreting magnetar?
文献类型：期刊论文
| 作者 | Tong, H.
|
| 刊名 | ASTRONOMISCHE NACHRICHTEN
 |
| 出版日期 | 2015-11-01 |
| 卷号 | 336期号:8-9页码:835-839 |
| 关键词 | accretion accretion disks pulsars: general stars: neutron |
| 英文摘要 | Magnetars are a special kind of neutron stars. There may also be accreting magnetars. From the studies of isolated magnetars, it is known that a neutron star with a strong dipole field only is not a magnetar. Super-slow X-ray pulsars may just be accreting high magnetic-field neutron stars. The ultra-luminous X-ray pulsar NuSTAR J095551+6940.8 may be an accreting magnetar. It may be an accreting low magnetic field magnetar with multipole field of 10(14) G and dipole field of 10(12) G. This point of view is consistent with the study of isolated magnetars. An ultra-luminous X-ray pulsar phase during binary evolution may result in massive millisecond pulsars. ((c) 2015 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim) |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | SOFT GAMMA-REPEATERS ; NEUTRON-STARS ; WIND BRAKING ; NUSTAR J095551+6940.8 ; RADIO PULSARS ; FIELD ; EMISSION ; BINARY ; M82 ; EVOLUTION |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000364913700021 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/897]  |
| 专题 | 脉冲星研究团组 新疆天文台_射电天文研究室 |
| 作者单位 | Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China |
| 推荐引用方式 GB/T 7714 | Tong, H.. Ultraluminous X-ray pulsar: Accreting magnetar?[J]. ASTRONOMISCHE NACHRICHTEN,2015,336(8-9):835-839. |
| APA | Tong, H..(2015).Ultraluminous X-ray pulsar: Accreting magnetar?.ASTRONOMISCHE NACHRICHTEN,336(8-9),835-839. |
| MLA | Tong, H.."Ultraluminous X-ray pulsar: Accreting magnetar?".ASTRONOMISCHE NACHRICHTEN 336.8-9(2015):835-839. |
入库方式： OAI收割
来源：新疆天文台
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