Table 2.
Parameters of the Milky Way models.
| Symbol | Parameter | Value |
|---|---|---|
| MMW | Disk mass | 1.3 × 1011 M⊙ |
| ad | Disk scale length | 5 kpc |
| bd | Disk scale length | 0.3 kpc |
| M* | Stellar disk mass | 5.51 × 1010 M⊙ |
| Mgas | Gas disk mass | 1.18 × 1010 M⊙ |
| R0* | Stellar disk scale length | 2.15 kpc |
| R0 gas | Gas disk scale length | 7 kpc |
| z0*, z0 gas | Stellar and gas disk scale height | 0.3 kpc |
Notes. Top half of table: parameters adopted for the Miyamoto-Nagai model (Eq. (13)), which we use to calculate the phantom dark matter profiles for the dwarf spheroidals. Bottom half of table: parameters used in Banik & Zhao (2018) for a realistic MOND Milky Way model, which includes exponential disks (see our Eqs. (14) and (15) for details). This second model is used here only for comparison to the Miyamoto-Nagai model (our Fig. 1) to show that our model is physically justified.
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