The role of environment in the evolution of disc galaxy density profiles - New insights from simulations and comparison to Euclid data

Open Access

Table 3.

Evolution of inner and outer slopes for initially Type IIprofiles.

Run	r_1 − 0	r_{1 − 1.5}	r_2 − 0	r_{2 − 1.5}
II-Wet-Control	2.79	2.83	0.83	1.04
II-Wet-Orb1	2.79	2.61	0.83	2.37
II-Wet-Orb2	2.79	2.57	0.83	2.87
II-Wet-Orb3	2.79	2.91	0.83	2.54
II-Wet-Orb4	2.79	2.63	0.83	2.39
II-Wet-Orb5	2.79	2.52	0.83	2.68
II-Wet-Orb6	2.79	2.65	0.83	2.39
II-Dry-Control	2.79	2.87	0.83	0.98
II-Dry-Orb1	2.79	2.76	0.83	1.91
II-Dry-Orb2	2.79	2.42	0.83	2.38

Notes.r_1 − 0 and r_{1 − 1.5} are the inner exponential scale lengths at 0 and 1.5 Gyr, measured between 1.5 and 6 kpc (to exclude the bulge and up to 90% of the break radius). r_2 − 0 and r_{2 − 1.5} are the outer scale lengths at the same epochs, measured between 7.5 and 10 kpc.

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.