中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
apossibleprecessingnozzleandthelensethirringeffectinblazar3c4543

文献类型:期刊论文

作者Qian Shanjie1; Britzen S2; Witzel A2; Krichbaum T P2; Gan Hengqian1; Gao Long1
刊名researchinastronomyandastrophysics
出版日期2014
卷号14期号:3页码:249
ISSN号1674-4527
英文摘要The kinematics of superluminal components in blazar 3C 454.3 are studied. Nine components are included: superluminal knots R1, R2, R3, R4, A, B, C and D (from Britzen et al. 2013) and C4 (from Pauliny-Toth 1998). We find that their kinematics derived from VLBI observations can be consistently interpreted in terms of a jet precession scenario with a period of about 14.5 yr. We discuss the model fits of their trajectory, distance from the core and apparent velocity. We show that the bulk Lorentz factor (in the range 4 to 15) derived for these components does not have any dependence on the phase of the precession (or position angle for ejection). The Lense-Thirring effect is assumed to interpret the precession of the jet nozzle. The results obtained for blazar 3C 454.3 are only suggestive. They are not unique and have yet to be tested, but they might be useful for understanding the kinematics of superluminal components in blazars and for disentangling different mechanisms and factors.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/52212]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.Max-Planck Institut fur Radioastronomie
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GB/T 7714
Qian Shanjie,Britzen S,Witzel A,et al. apossibleprecessingnozzleandthelensethirringeffectinblazar3c4543[J]. researchinastronomyandastrophysics,2014,14(3):249.
APA Qian Shanjie,Britzen S,Witzel A,Krichbaum T P,Gan Hengqian,&Gao Long.(2014).apossibleprecessingnozzleandthelensethirringeffectinblazar3c4543.researchinastronomyandastrophysics,14(3),249.
MLA Qian Shanjie,et al."apossibleprecessingnozzleandthelensethirringeffectinblazar3c4543".researchinastronomyandastrophysics 14.3(2014):249.

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来源:国家天文台

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