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Table 1.
Simulations for QUMOND.
| γ | Bulge | Hot gaseous halo | Number of stars |
|---|---|---|---|
| 1 | Spherical | No | 40 000 |
| 1 | Triaxial | No | Individual stars |
| 2 | Spherical | No | 40 000 |
| 2 | Triaxial | No | Individual stars |
| 1 | Spherical | Yes | 40 000 |
| 2 | Spherical | Yes | 40 000 |
Notes. To find the upper limit of |vϕ| for QUMOND with a triaxial bulge, we performed many simulations of individual stars. In this case, we used the gravitational field of the triaxial bulge within 5 kpc of the Galactic center and that of the spherical bulge at larger radii.
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