Milky Way: New Galactic mass model for orbit computations
Jozef Kla\v{c}ka, Michal \v{S}turc, Emil Puha

TL;DR
This paper develops a new Galactic mass model for the Milky Way by coupling an improved baryonic matter model with a dark matter distribution based on McGaugh et al.'s interpolating function, validated against observational data.
Contribution
It introduces a novel Galactic mass model combining refined baryonic matter and dark matter distributions, enhancing orbit computation accuracy for the Milky Way.
Findings
Rotation curve matches observational data
Tully-Fisher relation is satisfied
Key MW parameters are precisely estimated
Abstract
Accurate observational data on the rotation curve of the Milky Way galaxy (MW) are very well understood using the gravitational potentials of the baryonic matter (Pouliasis et al., 2017) and the interpolating function presented by McGaugh et al. (2016). In this way we couple the spherically symmetric mass distribution of the dark matter (DM) to the mass distribution of the baryonic matter (BM). A commonly used model of the dark matter distribution can be understood as an approximation of our model. Creation of a new Galactic mass model for orbit computations based on the coupling of the DM with an improved BM model respecting the theoretical fit of the Galactic rotation curve. The theoretical approach is based on a slight improvement of the BM model by Pouliasis et al. (2017) and on replacement of their DM model by the model based on the interpolating function by McGaugh et al. (2016).…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Scientific Research and Discoveries
