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Table 2
Best fit parameters for the four different Galactic stellar distribution models resulting from removing the data that is affected by known halo substructures (the Sagittarius stream and the anticentre substructures).
Model |
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ρ0 (pc-3) × 10-3 | Rbreak (kpc) | n | nin | nout | q | qin | qout | w |
|
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Axisymmetric | 1.90 | 14 ± 6 | – | −4.31 ± 0.09 | – | – | 0.79 ± 0.06 | – | – | – |
Triaxial | 1.86 | 14 ± 6 | – | −4.28 ± 0.09 | – | – | 0.77 ± 0.06 | – | – | 0.87 ± 0.09 |
Broken p.l.n | 1.52 | 0.071 ± 0.003 | 19.0 ± 0.5 | – | −2.40 ± 0.05 | −4.80 ± 0.05 | 0.77 ± 0.03 | – | – | – |
Broken p.l.n, q | 1.99,1.51 | 1 ± 3 | 19fixed | – | −3.3 ± 0.6 | −4.9 ± 0.2 | – | 0.7 ± 0.2 | 0.88 ± 0.07 | – |
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Initial parameters | – | 0.001 | 40.0 | −3.00 | −3.00 | −3.50 | 0.70 | 0.70 | 0.8 | 1.00 |
Notes. For the fitting, the data has been binned in 0.2 mag distance modulus cells.
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