Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation

LEO's

Nature Astronomy, Published online: 19 February 2024; doi:10.1038/s41550-024-02209-8

A dynamical model using the spatially resolved kinematics of galaxies in the CALIFA survey shows that galaxy assembly depends on both the stellar mass and the dynamical mass (which includes stars plus dark matter).

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