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Table 3

Characteristic times and merger-feature time to final coalescence time ratio.

Simulation tFP (Gyr)a tMS (Gyr)b tFC (Gyr)c tMF,25 (Gyr)d tMF,28 (Gyr)e tMF,25/tFCf tMF,28/tFCg

Equal-mass mergers in isolated environment
SbSb0p 0.41 0.71 1.07 2.43 ± 0.34 6.65 ± 0.66 2.27 ± 0.32 6.22 ± 0.62
SbSb45p 0.41 0.65 1.07 2.31 ± 0.15 7.52 ± 0.74 2.16 ± 0.14 7.03 ± 0.69
SbSb90p 0.41 0.76 1.30 3.37 ± 0.15 5.70 ± 0.45 2.59 ± 0.11 4.38 ± 0.34
SbSb135p 0.41 0.60 1.13 2.44 ± 0.12 6.13 ± 0.84 2.16 ± 0.10 5.43 ± 0.84
SbSb180p 0.41 0.65 1.03 2.10 ± 0.24 5.41 ± 0.42 2.04 ± 0.24 5.25 ± 0.41
SaSb45p 0.41 0.67 1.09 2.40 ± 0.33 5.63 ± 0.65 2.20 ± 0.30 5.17 ± 0.59
SaSb90p 0.41 0.90 1.41 2.59 ± 0.22 4.82 ± 0.25 1.83 ± 0.16 3.42 ± 0.18
SaSb135p 0.41 0.63 1.08 2.26 ± 0.20 4.99 ± 0.24 2.09 ± 0.19 4.62 ± 0.22
SbSb45r 0.38 0.51 0.73 2.25 ± 0.26 7.01 ± 0.26 3.08 ± 0.35 9.60 ± 0.35
SbSb45p+ 0.43 1.00 1.93 3.04 ± 0.18 6.69 ± 0.32 1.58 ± 0.09 3.47 ± 0.17
SbSb45e 0.49 0.61 0.84 2.68 ± 0.32 > 8.50 h 3.19 ± 0.38 > 10.12
SbSb45h 0.35 0.80 1.57 2.99 ± 0.20 5.60 ± 0.47 1.90 ± 0.13 3.57 ± 0.30

Mean 0.41± 0.03 0.71 ± 0.14 1.19 ± 0.33 2.57 ± 0.82 6.22 ± 1.73 2.16 ± 0.80 5.24 ± 1.46

Unequal-mass mergers in isolated environment
SbSb345h 0.44 1.11 2.13 4.59 ± 0.17 7.26 ± 0.66 2.15 ± 0.08 3.41 ± 0.31
SbSb645h 0.47 1.48 3.75 5.80 ± 0.14 8.30 ± 0.39 1.55 ± 0.04 2.21 ± 0.11
SbSb1045h 0.48 2.8 12.9

Meani 0.46± 0.02 1.30 ± 0.26 2.94 ± 1.15 5.19 ± 0.44 7.78 ± 0.77 1.77 ± 0.15 2.65 ± 0.26

Merger in a cluster potential
SbSb45hC 0.35 0.80 1.57 2.81 ± 0.17 4.02 ± 0.17 1.79 ± 0.11 2.56 ± 0.04

Notes.

(a)

First passage time.

(b)

Maximum separation time.

(c)

Final coalescence time.

(d)

Merger-feature time based on μr,limit = 25 mag arcsec-2.

(e)

Merger-feature time based on μr,limit = 28 mag arcsec-2.

(f)

Ratio between merger-feature time to final coalescence time based on μr,limit = 25 mag arcsec-2.

(g)

Ratio between merger-feature time to final coalescence time timescales based on μr,limit = 28 mag arcsec-2.

(h)

Disturbed structures are clearly visible until the end of simulation (8.5 Gyr).

(i)

In this case, we consider only SbSb345h and SbSb645h mergers.

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