Non-thermal pulsed X-ray emission from rotation-powered pulsars | |
Zhang L(张力)1,2; Jiang, ZJ2 | |
刊名 | ASTRONOMY & ASTROPHYSICS |
2006-08 | |
卷号 | 454期号:2页码:537-542 |
关键词 | pulsars : general radiation mechanisms : non-thermal X-rays : stars |
ISSN号 | 0004-6361 |
通讯作者 | Zhang, L (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming, Peoples R China. |
产权排序 | 第一完成单位 |
英文摘要 | We study the properties of the pulsed component of hard (> 2 keV) X-ray emission from pulsars based on the new version of the outer-gap model proposed by Zhang et al. (2004). In this outer-gap model, high-energy photons emitted by relativistic charged particles produce e(+/-) pairs through magnetic-pair production on their way from the outer gap to the neutron-star surface, and these pairs produce the bulk of pulsed X-rays by the synchrotron radiation. The X-ray luminosity of rotation-powered pulsars is a function not only of the period and magnetic field strength, but also of the magnetic inclination angle. Application of this model to the observed pulsed X-ray emission of normal pulsars by ASCA shows a better consistence. Further, the inclination angles of these pulsars are estimated using the observed X-ray data, and the predicted conversion efficiencies of high-energy gamma-rays for seven confirmed gamma-ray pulsars are consistent with the observed data. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | OUTER GAP ACCELERATOR ; ELECTRIC-FIELD STRUCTURE ; GAMMA-RAY ; NEUTRON-STARS ; LUMINOSITY ; SPECTRUM ; MODEL ; YOUNG ; RADIATION ; LOCATION |
收录类别 | SCI ; EI |
原文出处 | http://www.aanda.org/10.1051/0004-6361:20052758 |
语种 | 英语 |
WOS记录号 | WOS:000239004300044 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4201] |
专题 | 云南天文台_其他 |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming, China 2.Department of Physics, Yunnan University, Kunming, China |
推荐引用方式 GB/T 7714 | Zhang L,Jiang, ZJ. Non-thermal pulsed X-ray emission from rotation-powered pulsars[J]. ASTRONOMY & ASTROPHYSICS,2006,454(2):537-542. |
APA | Zhang L,&Jiang, ZJ.(2006).Non-thermal pulsed X-ray emission from rotation-powered pulsars.ASTRONOMY & ASTROPHYSICS,454(2),537-542. |
MLA | Zhang L,et al."Non-thermal pulsed X-ray emission from rotation-powered pulsars".ASTRONOMY & ASTROPHYSICS 454.2(2006):537-542. |
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