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What is MIGHTEE-HI Radial Acceleration Relation about?
This study presents a new measurement of the radial acceleration relation (RAR) using a homogeneous sample of Hi-selected galaxies, which links baryonic and dark matter by relating observed acceleration to baryonic mass. The authors introduce a novel method for measuring resolved stellar masses through spectral energy distribution fitting, revealing a tight RAR with a low-acceleration power-law slope of approximately 0.5 and minimal intrinsic scatter. The findings suggest the importance of resolved stellar
- Author
- videopaylasim05
- Language
- EN