Exploring Milky Way rotation curves with Gaia DR3: a comparison between $\Lambda$CDM, MOND, and General Relativistic approaches
With the release of Gaia DR3, we extend the comparison between dynamical models for the Milky Way rotation curve initiated in the previous work. Utilising astrometric and spectro-photometric data for 719143 young disc stars within $|z|
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Zusammenfassung: | With the release of Gaia DR3, we extend the comparison between dynamical
models for the Milky Way rotation curve initiated in the previous work.
Utilising astrometric and spectro-photometric data for 719143 young disc stars
within $|z| |
---|---|
DOI: | 10.48550/arxiv.2407.12482 |