Galaxy formation with local photoionization feedback - II. Effect of X-ray emission from binaries and hot gas

Galaxy formation with local photoionization feedback - II. Effect of X-ray emission from binaries and hot gas

We study how X-rays from stellar binary systems and the hot intracluster medium (ICM) affect the radiative cooling rates of gas in galaxies. Our study uses a novel implementation of gas cooling in the moving-mesh hydrodynamics code arepo. X-rays from stellar binaries do not affect cooling at all as...

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Bibliographic Details
Main Authors: Stinson, G. S. (Author), Hennawi, J. F. (Author), Springel, V. (Author), Macciò, A. V. (Author), Kannan, Rahul (Contributor), Vogelsberger, Mark (Contributor), Marinacci, Federico (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Oxford University Press, 2017-04-28T17:41:10Z.
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