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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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