Large scale mass_distribution_in_the_illustris_simulation

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MNRAS (2016) doi:10.1093/mnras/stw077
Large-scale mass distribution in the Illustris simulation
M. Haider,1‹
D. Steinhause...

2 M. Haider et al.
energies hint at large reservoirs of hot gas around spiral galax-
ies (Gupta et al. 2012), approximatel...

Large-scale mass distribution 3
Table 1. Mass fraction of dark matter and baryons inside haloes at z = 0. The mass fractio...

4 M. Haider et al.
Figure 2. Redshift evolution of the mass inside haloes. The values for dark
matter and baryons are norm...

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Large-scale mass distribution 5
Figure 3. Dark matter and baryon density in a thin slice at z = 0. The slice covers the wh...

6 M. Haider et al.
Figure 5. Redshift evolution of the baryon density. The same slice as in Fig. 3 has been used.
Figure 6...

Large-scale mass distribution 7
Figure 7. Baryon and dark matter mass distribution with respect to the dark matter density...

8 M. Haider et al.
Figure 9. Temperature ﬁeld of the gas in the slice of Fig. 3. We see that the
gas forms hot bubbles aro...

Large-scale mass distribution 9
Figure 12. Redshift evolution of the contribution of haloes, voids and ﬁlaments to the tot...

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10 M. Haider et al.
haloes deﬁned by a dark matter density cut. This suggests that
our method of measuring the mass using ...

Large-scale mass distribution 11
Le Brun et al. (2014) is very low compared to Illustris, which could
lead to different de...

12 M. Haider et al.
Nicastro F., Elvis M., Fiore F., Mathur S., 2005, Adv. Space Res., 36, 721
Nicastro F. et al., 2013, A...

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