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Table 2
Stellar mass distribution models of the Milky Way used in this Paper.
| Model 1 | Model 2 (fiducial) | |
|---|---|---|
| Nuclear star cluster | Best-fitting model from Chatzopoulos et al. (2015) | Best-fitting model from Chatzopoulos et al. (2015) |
| Nuclear stellar disc | Model 3 of Sormani et al. (2020a) | Fiducial model of Sormani et al. (2022b) |
| Galactic bar | Best-fitting model of Launhardt et al. (2002) | Bar + long bar from Sormani et al. (2022a) |
| Galactic disc | Best-fitting model of thin+thick disc from McMillan (2017) | Disc from Sormani et al. (2022a) |
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