Investigating the H I distribution and kinematics of ESO444-G084 and [KKS2000]23: New insights from the MHONGOOSE survey

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Table 8.

Best-fit dark matter halo parameters for ESO444–G084 and [KKS2000]23.

Galaxy	(M/L)^*	r_c (kpc)	ρ₀ (10⁻³ M_⊙ pc⁻³)	$χ_{red}^{2}$ $\chi _{\mathrm {red}}^2$	M_halo(<r) (10⁹ M_⊙)
ESO444–G084	0.2	3.48±0.57	16.05±1.45	2.6	2.23±0.17
ESO444–G084	0.5	5.84±2.64	11.47±1.46	4.3	2.12±0.45

[KKS2000]23	0.18	5.49±0.60	4.29±0.43	3.4	7.73±0.74
[KKS2000]23	0.5	7.11±0.86	3.30±0.30	3.06	7.91±1.20

Notes. Notes: The core radius (r_c) and central density (ρ₀) are derived for different (M/L)^* assumptions. The enclosed halo mass M_halo(<r) is computed within the last measured point of the rotation curve.

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