Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set
We use data from the Gaia DR3 data set to estimate the mass of the Milky Way (MW) by analyzing the rotation curve in the range of distances 5 to 28 kpc. We consider three mass models: The first model adds a spherical dark matter (DM) halo, following the Navarro-Frenk-White (NFW) profile, to the known stellar components. The second model assumes
Sylos Labini, Francesco et al.
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2023