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galpy: A python Library for Galactic Dynamics

  • Authors: Jo Bovy

Bovy 2015 The Astrophysical Journal Supplement Series 216 29.

  • Provider: AAS Journals

Caption: Figure 25.

Methods of quasiisothermaldf instances, illustrated using a MWPotential2014 potential, with Σ(R)∝exp [ − R/(R0/3)], σR(R) = 0.2 exp [ − (R − R0)/R0], and σz(R) = 0.1 exp [ − (R − R0)/R0]. Other marginalizations similar to df.pvRvT and df.pvz are available as well.

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