Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG

Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG

We study the connection between active galactic nuclei (AGN) and their host galaxies through cosmic time in the large-scale cosmological IllustrisTNG simulations. We first compare BH properties, i.e. the hard X-ray BH luminosity function, AGN galaxy occupation fraction, and distribution of Eddington...

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Váldodahkkit: Habouzit, Mélanie, Genel, Shy, Somerville, Rachel S, Kocevski, Dale, Hirschmann, Michaela, Dekel, Avishai, Choi, Ena, Nelson, Dylan, Pillepich, Annalisa, Hernquist, Lars, Vogelsberger, Mark, Weinberger, Rainer, Springel, Volker, Torrey, Paul A.
Eará dahkkit: Massachusetts Institute of Technology. Department of Physics
Materiálatiipa: Artihkal
Giella:English
Almmustuhtton: Oxford University Press (OUP) 2019
Liŋkkat:https://hdl.handle.net/1721.1/121487

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https://hdl.handle.net/1721.1/121487

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