Evolution of the disky second generation of stars in globular clusters on cosmological timescales

Open Access

Table 2

Initial kinematical and physical characteristics of GCs at T = −8 Gyr.

Pot.	Orbit	X	Y	Z	V_x	V_y	V_z
		pc	pc	pc	km s⁻¹	km s⁻¹	km s⁻¹
TNG	CR	4	7108	−871	189	−39	28
	TB	−1493	−3213	398	5	−3	−57
	LR	3597	13 451	−3767	−43	−167	23
FIX	CR	6725	413	498	−30	−201	25
	TB	566	265	-602	170	139	−104
	LR	−16 851	−4979	7933	23	8	12
ISO	–	0	0	0	0	0	0

Notes. Initial conditions (King models with W₀ = 9.0) for our theoretical GC models: M = 1.5 × 10⁵ M_⊙ with corresponding particle numbers N = 261 384 and half-mass radius r_hm = 2.0 pc.

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