Table 2.
Structural properties of the two clusters.
| # members | z | e | σlos | M⋆, tot | M200 | r200 | Rhm | TD | |
|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
| AS1063 | 1215 | 0.35 | 0.77 | 1350 km s−1 | 7.32 × 1013 M⊙ | 2.17 × 1015 M⊙ | 2.70 Mpc | 1.98 Mpc | 2 × 103 Gyr |
| M1206 | 658 | 0.44 | 0.75 | 1120 km s−1 | 5.38 × 1013 M⊙ | 1.40 × 1015 M⊙ | 1.97 Mpc | 1.21 Mpc | 7 × 102 Gyr |
Notes. (1) Number of member galaxies for which the position in the sky, velocity along the line of sight, and stellar mass are available. (2) Average cluster redshift z, based on the values of the redshift of the selected member galaxies. (3) Adopted eccentricity, as defined in the text (see Sect. 3). (4) Global velocity dispersion, based on the velocity distribution shown in Fig. 2. (5) Total stellar mass M⋆, tot associated with the distribution illustrated in Fig. 3. (6) Virial mass M200 and (7) virial radius r200, taken from Sartoris et al. (2020) for AS1063 and from Biviano et al. (2013) for M1206. (8) Half-mass radius Rhm, defined as the circularized radius that encloses half of the stellar mass projected on the sky. (9) Relaxation time TD, as defined in Eq. (1).
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