Table 1.

Pressure-supported Local Group dwarfs with globular clusters and velocity dispersion measurements.

NameTypeMVM*|$M_{\rm H\, {\small I}}$|Reσlog M200NGCMGCGC Ref
(mag)(107 M|$\odot$|)(107 M|$\odot$|)(pc)(km s−1)(M|$\odot$|)(104 M|$\odot$|)
SagittariusdSph−15.513.22587 (219)11.4 (0.7)10.788278L10
FornaxdSph−13.42.00.017710 (70)11.8 (0.2)9.06573M03
Eridanus IIdSph−7.10.0059280 (28)6.9 (1.1)9.0510.4Cr16
NGC 205dE−16.534.00.040590 (31)35.0 (5.0)9.8311140D88
NGC 185dE−14.87.10.011458 (45)24.0 (1.0)10.64868V13
NGC 147dE−14.65.9623 (62)16.0 (1.0)9.2710130V13
And IdSph−11.70.40672 (69)10.6 (1.1)9.2810.37C17
And XXVdSph−9.70.065642 (75)3.0 (1.0)7.1211.5Cu16
NameTypeMVM*|$M_{\rm H\, {\small I}}$|Reσlog M200NGCMGCGC Ref
(mag)(107 M|$\odot$|)(107 M|$\odot$|)(pc)(km s−1)(M|$\odot$|)(104 M|$\odot$|)
SagittariusdSph−15.513.22587 (219)11.4 (0.7)10.788278L10
FornaxdSph−13.42.00.017710 (70)11.8 (0.2)9.06573M03
Eridanus IIdSph−7.10.0059280 (28)6.9 (1.1)9.0510.4Cr16
NGC 205dE−16.534.00.040590 (31)35.0 (5.0)9.8311140D88
NGC 185dE−14.87.10.011458 (45)24.0 (1.0)10.64868V13
NGC 147dE−14.65.9623 (62)16.0 (1.0)9.2710130V13
And IdSph−11.70.40672 (69)10.6 (1.1)9.2810.37C17
And XXVdSph−9.70.065642 (75)3.0 (1.0)7.1211.5Cu16

Note. The top half of the table lists dwarfs associated with the Milky Way and the lower half with the Andromeda galaxy. Absolute magnitude (MV), stellar mass (M*), H i gas mass (⁠|$M_{\rm H\, {\small I}}$|⁠), half-light radius (Re), and central velocity dispersion (σ) are taken from the compilation of McConnachie (2012) and online updates. M/LV = 1 is used to calculate stellar mass. For Sagittarius see text for details. For Eridanus II data come from the discovery paper. The number of GCs (NGC) is taken from the GC reference: L10 – Law & Majewski (2010); M03 – Mackey & Gilmore (2003); Cr16 – Crnojević et al. (2016); D88 – Da Costa & Mould (1988); V13 – Veljanoski et al. (2013); C17 – Caldwell et al. (2017); and Cu16 – Cusano et al. (2016). See text for details of how the GC system mass (MGC) and halo mass (M200) are calculated. The online version of this table includes errors on the halo mass.

Table 1.

Pressure-supported Local Group dwarfs with globular clusters and velocity dispersion measurements.

NameTypeMVM*|$M_{\rm H\, {\small I}}$|Reσlog M200NGCMGCGC Ref
(mag)(107 M|$\odot$|)(107 M|$\odot$|)(pc)(km s−1)(M|$\odot$|)(104 M|$\odot$|)
SagittariusdSph−15.513.22587 (219)11.4 (0.7)10.788278L10
FornaxdSph−13.42.00.017710 (70)11.8 (0.2)9.06573M03
Eridanus IIdSph−7.10.0059280 (28)6.9 (1.1)9.0510.4Cr16
NGC 205dE−16.534.00.040590 (31)35.0 (5.0)9.8311140D88
NGC 185dE−14.87.10.011458 (45)24.0 (1.0)10.64868V13
NGC 147dE−14.65.9623 (62)16.0 (1.0)9.2710130V13
And IdSph−11.70.40672 (69)10.6 (1.1)9.2810.37C17
And XXVdSph−9.70.065642 (75)3.0 (1.0)7.1211.5Cu16
NameTypeMVM*|$M_{\rm H\, {\small I}}$|Reσlog M200NGCMGCGC Ref
(mag)(107 M|$\odot$|)(107 M|$\odot$|)(pc)(km s−1)(M|$\odot$|)(104 M|$\odot$|)
SagittariusdSph−15.513.22587 (219)11.4 (0.7)10.788278L10
FornaxdSph−13.42.00.017710 (70)11.8 (0.2)9.06573M03
Eridanus IIdSph−7.10.0059280 (28)6.9 (1.1)9.0510.4Cr16
NGC 205dE−16.534.00.040590 (31)35.0 (5.0)9.8311140D88
NGC 185dE−14.87.10.011458 (45)24.0 (1.0)10.64868V13
NGC 147dE−14.65.9623 (62)16.0 (1.0)9.2710130V13
And IdSph−11.70.40672 (69)10.6 (1.1)9.2810.37C17
And XXVdSph−9.70.065642 (75)3.0 (1.0)7.1211.5Cu16

Note. The top half of the table lists dwarfs associated with the Milky Way and the lower half with the Andromeda galaxy. Absolute magnitude (MV), stellar mass (M*), H i gas mass (⁠|$M_{\rm H\, {\small I}}$|⁠), half-light radius (Re), and central velocity dispersion (σ) are taken from the compilation of McConnachie (2012) and online updates. M/LV = 1 is used to calculate stellar mass. For Sagittarius see text for details. For Eridanus II data come from the discovery paper. The number of GCs (NGC) is taken from the GC reference: L10 – Law & Majewski (2010); M03 – Mackey & Gilmore (2003); Cr16 – Crnojević et al. (2016); D88 – Da Costa & Mould (1988); V13 – Veljanoski et al. (2013); C17 – Caldwell et al. (2017); and Cu16 – Cusano et al. (2016). See text for details of how the GC system mass (MGC) and halo mass (M200) are calculated. The online version of this table includes errors on the halo mass.

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