Abstract
We introduce a novel orbit superposition method designed to reconstruct the stellar density structure, kinematics, and chemical abundance distribution of the entire Milky Way by leveraging 6D phase-space information from its resolved stellar populations, limited by the spatial coverage of APOGEE DR17.
Original language | English |
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Journal | Astronomy & Astrophysics |
Publication status | Published - 1 Nov 2024 |
Austrian Fields of Science 2012
- 103003 Astronomy
- 103004 Astrophysics
Keywords
- Astrophysics - Astrophysics of Galaxies