Free Access

Table 2

Masses, scalelengths, scaleheights, and number of particles of the different components in the progenitor galaxies.

Characteristic parameters gE0 gS0 gSa gSb gSd dE0 dS0 dSa dSb dSd

(a) MBulge [2.3 × 109 M] 70 10 10 5 0 7 1 1 0.5 0
MHalo [2.3 × 109 M] 30 50 50 75 75 3 5 5 7.5 7.5
rBulge [kpc] 4 2 2 1 1.3 0.6 0.6 0.3
rHalo [kpc] 7 10 10 12 15 2.2 3.2 3.2 3.8 4.7

(b) M,Disc [2.3 × 109 M] 0 40 40 20 25 0 4 4 2 2.5
M g,Disc / M ,Disc 0 0 0.1 0.2 0.3 0 0 0.1 0.2 0.3
a,Disc [kpc] 4 4 5 6 1.3 1.3 1.6 1.9
h,Disc [kpc] 0.5 0.5 0.5 0.5 0.16 0.16 0.16 0.16
ag,Disc [kpc] 5 6 7 1.6 1.9 2.2
hg,Disc [kpc] 0.2 0.2 0.2 0.06 0.06 0.06

(c) N hybrid 20 000 40 000 60 000 8000 16 000 24 000
N stellar 80 000 320 000 60 000 40 000 20 000 32 000 32 000 24 000 16 000 8000
N DM 40 000 160 000 40 000 40 000 40 000 16 000 16 000 16 000 16 000 16 000

Notes. Rows: (a) Plummer sphere parameters used to model the bulges and haloes of the progenitor galaxies, as a function of the considered morphological types: MBulge is the (stellar) mass of the bulge, MHalo is the total mass of the dark matter halo, while rBulge and rHalo are their corresponding effective radii. (b) Parameters of the Miyamoto-Nagai density profiles used to model the gaseous and stellar discs of the different progenitors: the sub-index denotes the stellar disc, and the sub-index g refers to the gaseous disc, M is mass, a is effective radius, and h is the vertical scalelength. (c) Number of hybrid particles (initially fully gaseous), collisionless stellar particles, and dark matter particles used for each progenitor galaxy.

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.