| High-energy nonthermal emission from high-field pulsars | |
Zhang L(张力)1,2 ; Jiang, ZJ2; Zhang, L (reprint author), Natl Astron Observ, Yunnan Observ, Chinese Acad Sci, POB 110, Kunming 650011, Peoples R China.
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| 发表期刊 | ASTROPHYSICAL JOURNAL
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| 2005-10-10 | |
| 卷号 | 632期号:1页码:523-530 |
| DOI | 10.1086/432595 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI |
| 关键词 | Gamma Rays : Theory Pulsars : General Radiation Mechanisms : Nonthermal X-rays : Stars |
| 摘要 | We study high-energy radiation properties of high-field (10(13)-10(14)G) pulsars in the framework of the outer-gap model. In this model, charged particles are accelerated inside the outer gap, which depends on the magnetic inclination angle and magnetic geometry. High-energy photons emitted by these relativistic charged particles produce electrons/positrons through magnetic pair production on their way from the outer gap to the neutron star surface, and these pairs produce nonthermal X-rays by synchrotron radiation. Applying this model to high- field pulsars, the characteristic gamma-ray energies, nonthermal X-ray luminosity, and gamma-ray luminosity are calculated. Furthermore, comparisons of the predicted gamma-ray fluxes for these high-field pulsars with the sensitivities of AGILE and GLAST are given. We discuss the possibility that some high-field pulsars with ages of similar to 10(4.9) to similar to 10(5.5) yr might be detected by AGILE. |
| 语种 | 英语 |
| 学科领域 | Astronomy & Astrophysics |
| 文章类型 | Article |
| ISSN | 0004-637X |
| URL | 查看原文 |
| 归档日期 | 2005-11-10 |
| WOS记录号 | WOS:000232366000037 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | GAMMA-RAY EMISSION ; RAPIDLY SPINNING PULSARS ; STRONGLY MAGNETIZED PLASMAS ; OUTER GAP ACCELERATOR ; POWERED NEUTRON-STARS ; X-RAY ; PSR B1509-58 ; RADIO PULSAR ; VACUUM POLARIZATION ; THERMAL EMISSION |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4185 |
| 专题 | 其他 |
| 通讯作者 | Zhang, L (reprint author), Natl Astron Observ, Yunnan Observ, Chinese Acad Sci, POB 110, Kunming 650011, Peoples R China. |
| 作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, China 2.Department of Physics, Yunnan University, Kunming 650091, China |
| 第一作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Zhang L,Jiang, ZJ,Zhang, L . High-energy nonthermal emission from high-field pulsars[J]. ASTROPHYSICAL JOURNAL,2005,632(1):523-530. |
| APA | Zhang L,Jiang, ZJ,&Zhang, L .(2005).High-energy nonthermal emission from high-field pulsars.ASTROPHYSICAL JOURNAL,632(1),523-530. |
| MLA | Zhang L,et al."High-energy nonthermal emission from high-field pulsars".ASTROPHYSICAL JOURNAL 632.1(2005):523-530. |
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| High-Energy Nontherm（219KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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