Mass distributions of star clusters for different star formation histories in a galaxy cluster environment

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Table 2

Duration of one SC formation epoch, δt, and the reduced as determined from the least-squares fits in Fig. 4 for each β (Col. 1).

β	δt		δt
	[Myr]		[Myr]

1.5	0.42	0.409	0.31	0.230
1.6	0.55	0.409	0.41	0.229
1.7	0.77	0.409	0.56	0.226
1.8	1.11	0.410	0.81	0.223
1.9	1.70	0.414	1.24	0.219
2.0	2.80	0.424	2.01	0.216
2.1	4.94	0.443	3.51	0.218
2.2	9.31	0.475	6.51	0.230
2.3	18.57	0.524	12.75	0.255
2.4	38.77	0.591	26.09	0.296
2.5	83.77	0.677	55.19	0.355
2.6	185.82	0.782	119.79	0.432

Notes. In Cols. 2 and 3 all data points are used while in Cols. 4 and 5 the four data points lying above the relation in Fig. 4 (with 10⁵M_⊙ ≲ M_ecl,max ≲ 10⁶M_⊙) are excluded. All values are visualized in Fig. 5.

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