Properties of the ionized CGM and IGM: tests for galaxy formation models from the Sunyaev–Zel’dovich effect

Properties of the ionized CGM and IGM: tests for galaxy formation models from the Sunyaev–Zel’dovich effect

We present a comparison of the physical properties of the ionized gas in the circumgalactic medium and intergalactic medium (IGM) at z ∼ 0 between observations and four cosmological hydrodynamical simulations: Illustris, TNG300 of the IllustrisTNG project, EAGLE, and one of the Magneticum simulation...

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Xehetasun bibliografikoak
Egile Nagusiak: Lim, SH, Barnes, D, Vogelsberger, M, Mo, HJ, Nelson, D, Pillepich, A, Dolag, K, Marinacci, F
Beste egile batzuk: MIT Kavli Institute for Astrophysics and Space Research
Formatua: Artikulua
Hizkuntza:English
Argitaratua: Oxford University Press (OUP) 2022
Sarrera elektronikoa:https://hdl.handle.net/1721.1/142410

Internet

https://hdl.handle.net/1721.1/142410

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