The evolution of an intra-cluster and intra-group stellar population - Their contribution to the stellar mass, their age, and their dynamics

Free Access

Table 1:

Properties of the particles in the simulations.
	Particle	Particle	Particle
	mass	mass	mass	length
	dark matter	gas	stellar	softening
	$M_{\hbox{$\odot$ }}$ h^-1	$M_{\hbox{$\odot$ }}$ h^-1	$M_{\hbox{$\odot$ }}$ h^-1	[kpc h^-1]
group	$1.5 \times 10^8$	$1.7 \times 10^7$	$7.8 \times 10^6$	4
cluster	$1.4 \times 10^8$	$1.7 \times 10^7$	$7.3 \times10^6$	4

Notes. Particle mass resolution and softening length for the simulations.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.