Institutional Repository of Radio Astronomy Research Laboratory
| PULSAR WIND MODEL FOR THE SPIN-DOWN BEHAVIOR OF INTERMITTENT PULSARS | |
Li, L.1,2,3 ; Tong, H.1; Yan, W. M.1; Yuan, J. P.1; Xu, R. X.4,5; Wang, N.1
| |
| 2014-06-10 | |
| Source Publication | ASTROPHYSICAL JOURNAL
 |
| Volume | 788Issue:1Pages:16 |
| Contribution Rank | 1 |
| Abstract | 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. |
| Correspondent Email | tonghao@xao.ac.cn |
| Keyword | Stars : Neutron Pulsars : Individual (Psr b1931+24 Psr j1832+0029 Psr J1841-0500) Stars : Winds Outflows |
| Subtype | Article |
| DOI | 10.1088/0004-637X/788/1/16 |
| WOS Headings | Science & Technology ; Physical Sciences |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | TIME RADIO PULSARS ; GAMMA-RAY EMISSION ; BRAKING INDEXES ; PAIR FORMATION ; ANTI-GLITCH ; POLAR CAPS ; MAGNETAR ; MAGNETOSPHERES ; STARS |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000337095200016 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/590 |
| Collection | 射电天文研究室_脉冲星研究团组 射电天文研究室 其它 |
| Corresponding Author | Tong, H. |
| Affiliation | 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 |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation 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. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Pulsar wind model fo（264KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-ND | View Application Full Text | |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment