Table 1.
Resulting parameters for models A, B, and C.
| Parameter | Model A | Model B | Model C |
|---|---|---|---|
| M* | 1.7 × 1011 M⊙ | 1.6 × 1011 M⊙ | 2.1 × 1011 M⊙ |
| Mvir | 3.4 × 1012 M⊙ | 5.4 × 1012 M⊙ | 2.5 × 1012 M⊙ |
| ra | 2.26 kpc | 2.7 kpc | 2.1 kpc |
| rb | 2.26 kpc | 2.26 kpc | – |
| rc | 2.54 kpc | 2.4 kpc | – |
| θ0 | −87.8° | −89° | – |
| λ0 | 112° | 114° | – |
| α | 60.6° | 54.9° | – |
| cvir | 7.4 | 7.4 | 7.4 |
| τ | 120 Myrs | 380 Myrs | – |
| iBulge | 61.7° | 63.8° | 62° |
| PABulge | 257° | 258° | 257° |
Notes. M* is the bulge stellar mass, ra, rb, and rc are the three axis scales and iBulge, PABulge is the orientation of the axis, c, relative to the observer. Mvir is the virial mass and cvir the concentration parameter of the dark matter. θ0 and λ0 are the starting values of the disk orientation. α is the dissipation settling angle and τ the time after the initial values.
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