Inflow and Outflow (Jets) in NGC 1275
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.
- Publication:
-
Perseus in Sicily: From Black Hole to Cluster Outskirts
- Pub Date:
- 2020
- DOI:
- Bibcode:
- 2020IAUS..342...69N
- Keywords:
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- galaxies: active;
- galaxies: individual (NGC 1275);
- galaxies: jets