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Inflow and Outflow (Jets) in NGC 1275

Published online by Cambridge University Press:  07 April 2020

Hiroshi Nagai
Hiroshi Nagai*
Affiliation:
National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo 1818-8588, Japan email: hiroshi.nagai@nao.ac.jp The Graduate University for Advanced Studies (SOKENDA), Osawa 2-21-1, Mitaka, Tokyo 1818-8588, Japan
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Abstract

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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.

Keywords

galaxies: activegalaxies: individual (NGC 1275)galaxies: jets
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S342: Perseus in Sicily: From Black Hole to Cluster Outskirts , May 2018 , pp. 69 - 72
Copyright
© International Astronomical Union 2020

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