NAOC Open IR
apossibleprecessingnozzleandthelensethirringeffectinblazar3c4543
Qian Shanjie1; Britzen S2; Witzel A2; Krichbaum T P2; Gan Hengqian1; Gao Long1
2014
Source Publicationresearchinastronomyandastrophysics
ISSN1674-4527
Volume14Issue:3Pages:249
AbstractThe 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.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/52213
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.Max-Planck Institut fur Radioastronomie
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
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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