Estimating the baryonic masses of face-on spiral galaxies from stellar kinematics
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DOI: 10.1093/mnras/stx917
Abstract: The kinematic dispersions of disc stars can be used to measure the dynamic contributions of baryons to the rotation curves of spiral galaxies and hence to trace the amount and distribution of the remaining dark… read more here.
Keywords: dark matter; spiral galaxies; kinematics; estimating baryonic ... See more keywords