Globular cluster orbital decay in dwarf galaxies with MOND and CDM: Impact of supernova feedback

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Table 2.

Parameters of the basic Newtonian models used to generate the initial conditions in PoR and MAGI.

Name	M_bar	r_D	q	f_gas	T	σ₀	Q_{R_D}
	[10⁸ M_⊙]	[kpc]			[K]	[ $\frac{kpc}{Myr}$ $\frac{\mathrm{kpc}}{\mathrm{Myr}}$ ]
GDw1e8N	1	0.8	0.4	0.9	23 000	5	1
GDw2e7N	0.2	0.5	0.4	0.9	23 000	0.3	1

Name	N_*	M_vir	r_s	r_trunc	w_trunc	M_h	N_h
	[10⁶]	[10⁹ M_⊙]	[kpc]	[kpc]	[kpc]	[10⁹ M_⊙]	[10⁶]
GDw1e8N	0.1	21	4.83	15	2	7.5	8
GDw2e7N	0.1	6.6	2.98	15	2	3.3	8

Notes. M_bar: Total baryonic mass. r_D: Disk scale length (the same for the stellar and gas disk). q: Axial ratio of the disk. f_gas: Gas fraction. T: Gas temperature. σ₀ and Q_{R_D}: Special parameters of the MAGI code (see Miki & Umemura 2018). N_*: Number of particles representing the stellar disk. M_vir: Virial mass of the NFW dark halo (if the halo were not truncated). r_s: Scale radius of the NFW dark halo. r_trunc: Truncation radius of the halo. w_trunc: Width of the truncation. M_h: Actual mass of the halo (after applying the truncation). N_h: Number of particles representing the halo.

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