The p-Laplacian as a framework for generalizing Newtonian gravity and Milgromian gravitation

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Table C.1.

Data on how Milky Way affects its dSphs via gravity.

Galaxy	$\frac{D_{host}}{kpc}$ $\frac {D_{\textrm {host}}}{{\mathrm {kpc}}}$	${log}_{10} (\frac{g_{host}}{{m s}^{- 2}})$ $\log _{10}(\frac {g_{\textrm {host}}}{{\mathrm {m\,s}}^{-2}})$	${log}_{10} (\frac{g_{N}}{{m s}^{- 2}})$ $\log _{10}(\frac {g_{\textrm {N}}}{{\mathrm {m\,s}}^{-2}})$	p
Carina	107	−10.91	−12.15±0.27	2.1±2.3
Draco	76	−10.62	−12.18±0.14	2.2±3.8
Fornax	149	−11.20	−11.35±0.17	2.2±1.1
Leo I	258	−11.68	−11.06±0.18	2.6±1.5
Leo II	236	−11.60	−11.67±0.26	2.8±2.3
Sculptor	86	−10.72	−11.48±0.26	2.1±3.0
Sextans	89	−10.75	−12.96±0.24	1.7±1.1
Ursa Minor	78	−10.64	−12.60±0.25	2.0±2.2
Bootes I	64	−10.47	−13.47±0.14	1.5±1.0
Bootes II	40	−10.06	−13.40±0.53	0±220
Canes V. I	216	−11.52	−13.40±0.14	2.40±0.41
Canes V. II	161	−11.27	−12.76±0.14	2.7±3.2
Coma B.	45	−10.16	−13.19±0.27	1.4±3.6
Hercules	128	−11.07	−12.92±0.22	2.0±1.6
Horologium I	79	−10.65	−12.78±0.17	3±49
Hydra II	131	−11.09	−12.88±0.28	3±16
Leo IV	155	−11.24	−13.30±0.30	2.1±3.1
Leo V	176	−11.35	−13.03±0.38	2.0±4.3
Leo T	422	−12.11	−11.70±0.14	4.0±6.3
Pisces II	195	−11.44	−12.91±0.29	4±27
Reticulum II	31	−9.84	−13.10±0.13	1±10
Segue I	28	−9.75	−13.22±0.45	1±21
Segue II	41	−10.08	−13.17±0.20	1±11
Tucana	883	−12.75	−11.98±0.21	20±140
Ursa Major I	101	−10.86	−13.27±0.27	2.6±4.3
Ursa Major II	38	−10.02	−13.49±0.23	1.2±6.8
Willman I	43	−10.12	−12.63±0.36	2±28

Notes. Columns from left to right: name of galaxy, distance, D_host, Milky Way and galaxy, Milky Way field, g_host, on galaxy, Newtonian field, g_N, of galaxy, p parameter obtained from g_host+g_N, D_host, g_N taken from Lelli et al. (2017), g_host calculated from Eq. (55), and p from Eq. (53).

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