NGC 1275: Baryonic cycing in the Perseus cluster of galaxies
Author:
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference27 articles.
1. Molecular gas in the Perseus cooling flow galaxy, NGC 1275
2. XMM‐NewtonObservations of the Perseus Cluster. I. The Temperature and Surface Brightness Structure
3. On the Nature of the NGC 1275 System
4. Donahue, M., Voit, G.M.: 2004, in: J.S. Mulchaey, A. Dressler, A. Oemler (eds.), Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution, p. 143
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1. Multiwavelength study of the radio galaxy NGC 1275 with TACTIC, Fermi and Swift during December, 2016 – February, 2017;New Astronomy;2020-10
2. TeV gamma-rays from the region of Perseus Cluster;Journal of Physics: Conference Series;2020-02-01
3. Origin of very high energy emission in galaxy clusters;EPJ Web of Conferences;2017
4. Very high energy gamma-ray emission of Perseus Cluster and NGC 1275;Journal of Physics: Conference Series;2016-07
5. Emission from the galaxy NGC 1275 at high and very high energies and its origin;Astronomy Letters;2014-02
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