Table 2.
Properties of the seven halos in the DMO run.
Halo ID | M200 | R1/2,init | R1/2,fin | σLOS, fin | # |
---|---|---|---|---|---|
[109 M⊙] | [pc] | [pc] | [km s−1] | ||
h277 | 0.49 | 28.99 | 96.86 | 4.02 | 3 |
h249 | 0.53 | 21.86 | 59.14 | 3.73 | 3 |
h315 | 0.42 | 14.21 | 53.48 | 3.03 | 2 |
h323 | 0.38 | 25.80 | 36.08 | 2.96 | 2 |
h170 | 0.83 | 20.29 | 89.34 | 4.41 | 5 |
h273 | 0.49 | 20.05 | 48.33 | 3.40 | 5 |
h291 | 0.49 | 34.82 | 77.82 | 3.40 | 2 |
Notes. R1/2,init is the half-mass radius of the dominant cluster at z = 6. R1/2,fin is the half-mass radius of the UFDs at z = 0, obtained through the contribution of all clusters. M200 is the virial mass. We note that it is systematically larger compared to the value derived from the hydro-runs (see Table 1). This is due to the fact that in the latter simulations, the gas has been lost at the end of the EoR. σLOS, fin is the line-of-sight velocities of clusters at z = 0. The last column gives the number of clusters found in each halo.
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