Age, local mass density ρ(r⊙,z⊙), disk axis ratio ϵ, and IMF of the different stellar components of the disks in the Besançon model. WD represents the white dwarfs.
|1–2||6.2×10-3||0.0375||dn/dm ∝ (m/M⊙)− α|
|2–3||4.0×10-3||0.0551||α = 1.6 for m< 1M⊙|
|3–5||5.8×10-3||0.0696||α = 3.0 for m> 1M⊙|
|Thick disk||all||1.64×10-3||dn/dm ∝ (m/M⊙)-0.5|
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