中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Formation of recollimation shocks in jets of high-mass X-ray binaries

文献类型:期刊论文

作者Yoon, DooSoo1,2; Zdziarski, Andrzej A.3; Heinz, Sebastian2
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2016-03-11
卷号456期号:4页码:3638-3644
ISSN号0035-8711
关键词Acceleration Of Particles Stars: Individual: Cyg X-1 Stars: Individual: Cyg X-3 Ism: Jets And Outflows X-rays: Binaries
DOI10.1093/mnras/stv2954
英文摘要We study conditions for formation of recollimation shocks in jets interacting with stellar winds in high-mass X-ray binaries. We show the existence of a critical jet power, dependent on the wind rate and velocity and the jet velocity, above which a recollimation shock is not formed. For jet powers below critical, we derive the location of the shock. We show that surface shocks may still exist above the critical power, but only occupy a small volume of the jet and do not significantly alter the jet opening angle. We test these prediction by 3D numerical simulations, which confirm the existence and the value of the critical power. We apply our results to Cyg X-1 and Cyg X-3.
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000372265800017
源URL[http://119.78.226.72/handle/331011/32835]  
专题中国科学院上海天文台
通讯作者Zdziarski, Andrzej A.
作者单位1.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
2.Univ Wisconsin, Dept Astron, Madison, WI 53706 USA
3.Ctr Astron M Kopernika, Bartycka 18, PL-00716 Warsaw, Poland
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Yoon, DooSoo,Zdziarski, Andrzej A.,Heinz, Sebastian. Formation of recollimation shocks in jets of high-mass X-ray binaries[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2016,456(4):3638-3644.
APA Yoon, DooSoo,Zdziarski, Andrzej A.,&Heinz, Sebastian.(2016).Formation of recollimation shocks in jets of high-mass X-ray binaries.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,456(4),3638-3644.
MLA Yoon, DooSoo,et al."Formation of recollimation shocks in jets of high-mass X-ray binaries".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 456.4(2016):3638-3644.

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