PULSAR WIND MODEL FOR THE SPIN-DOWN BEHAVIOR OF INTERMITTENT PULSARS
文献类型：期刊论文
| 作者 | Li, L.1,2,3 ; Tong, H.1; Yan, W. M.1; Yuan, J. P.1; Xu, R. X.4,5; Wang, N.1
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2014-06-10 |
| 卷号 | 788期号:1页码:16 |
| 通讯作者邮箱 | tonghao@xao.ac.cn |
| 关键词 | pulsars : individual (PSR B1931+24, PSR J1832+0029, PSR J1841-0500) stars : neutron stars : winds, outflows |
| 通讯作者 | Tong, H. |
| 英文摘要 | Intermittent pulsars are part-time radio pulsars. They have higher slow down rates in the on state (radio-loud) than in the off state (radio-quiet). This gives evidence that particle wind may play an important role in pulsar spindown. The effect of particle acceleration is included in modeling the rotational energy loss rate of the neutron star. Applying the pulsar wind model to the three intermittent pulsars (PSR B1931+24, PSR J1841-0500, and PSR J1832+0029) allows their magnetic fields and inclination angles to be calculated simultaneously. The theoretical braking indices of intermittent pulsars are also given. In the pulsar wind model, the density of the particle wind can always be the Goldreich-Julian density. This may ensure that different on states of intermittent pulsars are stable. The duty cycle of particle wind can be determined from timing observations. It is consistent with the duty cycle of the on state. Inclination angle and braking index observations of intermittent pulsars may help to test different models of particle acceleration. At present, the inverse Compton scattering induced space charge limited flow with field saturation model can be ruled out. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | TIME RADIO PULSARS ; GAMMA-RAY EMISSION ; BRAKING INDEXES ; PAIR FORMATION ; ANTI-GLITCH ; POLAR CAPS ; MAGNETAR ; MAGNETOSPHERES ; STARS |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000337095200016 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/590]  |
| 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.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 2.Univ Chinese Acad Sci, Beijing, Peoples R China 3.Xinjiang Univ, Sch Phys, Urumqi, Xinjiang, Peoples R China 4.Peking Univ, Sch Phys, Beijing 100871, Peoples R China 5.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China |
| 推荐引用方式 GB/T 7714 | Li, L.,Tong, H.,Yan, W. M.,et al. PULSAR WIND MODEL FOR THE SPIN-DOWN BEHAVIOR OF INTERMITTENT PULSARS[J]. ASTROPHYSICAL JOURNAL,2014,788(1):16. |
| APA | Li, L.,Tong, H.,Yan, W. M.,Yuan, J. P.,Xu, R. X.,&Wang, N..(2014).PULSAR WIND MODEL FOR THE SPIN-DOWN BEHAVIOR OF INTERMITTENT PULSARS.ASTROPHYSICAL JOURNAL,788(1),16. |
| MLA | Li, L.,et al."PULSAR WIND MODEL FOR THE SPIN-DOWN BEHAVIOR OF INTERMITTENT PULSARS".ASTROPHYSICAL JOURNAL 788.1(2014):16. |
入库方式： OAI收割
来源：新疆天文台
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