Chemical evolution models for the dwarf spheroidal galaxies Leo 1 and Leo 2

Free Access

Table 1:

Models with galactic winds for the dSph galaxies Leo 1 and Leo 2.
Galaxy	$\nu~({\rm Gyr}^{-1})$	w_i	n	t (Gyr)	d (Gyr)	$M_{\rm tot}$ (10⁷ $M_{\rm o}$ )	$M_{\rm gas}$ (10⁴ $M_{\rm o}$ )	IMF
Leo 1a	0.15	6	2	0/5	5/7	2.15	1.85	Salpeter
Leo 1b	0.60	9	2	0/5	5/7	4.06	1.97	Salpeter
Leo 1c	1.70	10	2	0/5	5/7	8.33	3.59	Salpeter
Leo 2a	0.05	2	1	0	7	2.12	3.67	Salpeter
Leo 2b	0.30	8	1	0	7	2.69	1.54	Salpeter
Leo 2c	1.50	11	1	0	7	7.03	2.68	Salpeter

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.