Impact of supernova feedback on the Tully-Fisher relation

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Table 1:

Cosmological hydrodynamical simulations studied in this paper.
Name	F/NF	$N_{\rm p}$	$M_{\rm dark}$	$M_{\rm gas}$
			$[10^6~ {M}_{\odot}~ h^{-1}]$	$[10^6~ {M}_{\odot}~ h^{-1}]$
S160	F	$2\times 160^3$	17.6	2.71
S230	F	$2 \times 230^3$	5.93	0.91
S230NF	NF	$2 \times 230^3$	5.93	0.91
S320	F	$2 \times 320^3$	2.20	0.34

Notes. Column 2: Model with/without SN feedback (F/NF). Column 3: Initial number of particles in the simulation. Column 4: Mass of dark matter particles. Column 5: Initial mass of gas particles.

Source LaTeX | All tables | In the text

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