Millimeter-VLBI observations of low-luminosity active galactic nuclei with source-frequency phase-referencing
2021-11-17
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摘要

We report millimeter-VLBI results of low-luminosity active galactic nuclei (M 84 and M 87) up to 88 GHz with source-frequency phase-referencing observations. We detected the weak VLBI core and obtained the first image of M 84 at 88 GHz. The derived brightness temperature of M 84 core was about 7.2×109 K, which could serve as a lower limit as the core down to 30 Schwarzschild radii was still un-resolved in our 88 GHz observations. We successfully determined the core-shifts of M 87 at 22-44 GHz and 44-88 GHz through source-frequency phase-referencing technique. The jet apex of M 87 could be deduced at ∼46 μas upstream of the 43 GHz core from core-shift measurements. The estimated magnetic field strength of the 88 GHz core of M 87 is 4.8 ± 2.4 G, which is at the same magnitude of 1-30 G near the event horizon probed by the Event Horizon Telescope.

关键词LLAGN M 84 M 87 — VLBI
DOIarXiv:2111.08930
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出处Arxiv
WOS记录号PPRN:12214624
WOS类目Astronomy& Astrophysics
资助项目National Natural Science Foundation of China[
文献类型预印本
条目标识符https://kms.shanghaitech.edu.cn/handle/2MSLDSTB/348524
专题物质科学与技术学院_博士生
作者单位
1.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
3.Univ Valencia, Dept Astron & Astrophys, E-46100 Burjassot, Spain
4.ShanghaiTech Univ, 393 Middle Huaxia Rd, Pudong, Shanghai 201210, Peoples R China
5.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
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Jiang, Wu,Shen, Zhiqiang,Marti-Vidal, Ivan,et al. Millimeter-VLBI observations of low-luminosity active galactic nuclei with source-frequency phase-referencing. 2021.
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