A possible feature of thermal matter in relativistic jets of radio-loud quasars
文献类型:期刊论文
作者 | Wang JM(王建民)![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2004 |
卷号 | 419期号:2页码:L9-L12 |
关键词 | galaxy : radio galaxies : active quasars individual : 3C 273 |
通讯作者 | Univ Tubingen, Inst Astron & Astrophys, Abt Astron, D-72076 Tubingen, Germany ; Chinese Acad Sci, Inst High Energy Phys, High Energy Astrophys Lab, Beijing 100039, Peoples R China ; INTEGRAL Sci Data Ctr, CH-1290 Versoix, Switzerland ; Observ Geneva, CH-1290 Sauverny, Switzerland |
英文摘要 | It has been suggested that relativistic jets in quasars may contain a considerable amount of thermal matter. In this paper, we explore the possibility that the Kalpha line from the thermal matter may appear at tens of keV due to a high Doppler blue-shift. In the jet comoving frame, the energy density of photons originally emitted by the accretion disk and reflected off the broad line region clouds dominates over that of photons of other origin. We discuss the photoionization states of the thermal matter and find that the irons elements are neutral. The high metallicity in quasars enhances the possibility to detect the thermal matter in the relativistic jet in some radio-loud quasars. A highly Doppler blue-shifted Kalpha line may be detected. We make a prediction for 3C 273, in which the Kalpha line luminosity might be of the order 3.0 x 10(44) erg s(-1) with an equivalent width of 2.4 keV. Such a line could be detected in a future mission. |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
原文出处 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000221886800002 |
源URL | [http://ir.ihep.ac.cn/handle/311005/240308] ![]() |
专题 | 高能物理研究所_粒子天体物理中心 |
作者单位 | 中国科学院高能物理研究所 |
推荐引用方式 GB/T 7714 | Wang JM,Wang, JM,Staubert, R,et al. A possible feature of thermal matter in relativistic jets of radio-loud quasars[J]. ASTRONOMY & ASTROPHYSICS,2004,419(2):L9-L12. |
APA | 王建民,Wang, JM,Staubert, R,&Courvoisier, TJL.(2004).A possible feature of thermal matter in relativistic jets of radio-loud quasars.ASTRONOMY & ASTROPHYSICS,419(2),L9-L12. |
MLA | 王建民,et al."A possible feature of thermal matter in relativistic jets of radio-loud quasars".ASTRONOMY & ASTROPHYSICS 419.2(2004):L9-L12. |
入库方式: OAI收割
来源:高能物理研究所
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