To reconstruct the history of the Milky Way, the chemo-physical characterization of stars is essential. For this, the chemical abundances of the Gaia Data Release 3 spectroscopy are of special importance, as they can be combined with dynamical properties in a chemo-kinematical analysis to find the relations between the chemistry and the Milky Way structure. This project explores nine abundance ratios in the DR3 and their evolution with the metallicity, distance to the galactic plane, azimuthal velocity, and eccentricity of the orbits of the stars.
| Identifer | oai:union.ndltd.org:UPSALLA1/oai:DiVA.org:uu-528279 |
| Date | January 2024 |
| Creators | Bellido Hacar, Isabel |
| Publisher | Uppsala universitet, Institutionen för fysik och astronomi |
| Source Sets | DiVA Archive at Upsalla University |
| Language | English |
| Detected Language | English |
| Type | Student thesis, info:eu-repo/semantics/bachelorThesis, text |
| Format | application/pdf |
| Rights | info:eu-repo/semantics/openAccess |
| Relation | FYSAST ; FYSPROJ1339 |
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