Inflow and Outflow (Jets) in NGC 1275
Inflow and Outflow (Jets) in NGC 1275
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DOI：
10.1017/s1743921318005744
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发表时间：
2018-05
期刊：
影响因子：
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通讯作者：
H. Nagai
中科院分区：
文献类型：
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作者：
H. Nagai
Abstract NGC 1275 is one of the best targets to study the high energy emission mechanism in radio galaxies and the accretion flow properties using a young re-started jet 3C 84 as a prober of subpc-to-pc scale environment. In this proceeding, we review the observation results from a series of our VLBI observations and discuss on the origin of gamma-ray emission and accretion flow properties. We also briefly present the preliminary results from our recent ALMA observations.
