Isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metalicity gradients

Free Access

Table 1:

Range of masses within which the simulations are run.
Total Mass $[M_{\odot}]$	from	to	$\gamma$
$M_{{\rm star}}$	$5.1 \times 10^4$	$1.0 \times 10^8$	$\gamma=1.5$
$M_{{\rm dark}}$	$7.1 \times 10^7$	$1.9 \times 10^9$	$\gamma \in [0.5,2]$
$M_{{\rm gas}}$	$5.5 \times 10^4$	$6.9 \times 10^6$	$\gamma=1.5$

Notes. The scale lengths refer to r₉₀ as discussed in the text. The values listed here are our starting values at the initial time T=T₀.

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.