The mass discrepancy acceleration relation in early-type galaxies: extended mass profiles and the phantom menace to MOND
The dark matter (DM) haloes around spiral galaxies appear to conspire with their baryonic content: empirically, significant amounts of DM are inferred only below a universal characteristic acceleration scale. Moreover, the discrepancy between the baryonic and dynamical mass, which is usually interpr...
| Váldodahkkit: | , , , , , |
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| Materiálatiipa: | Journal article |
| Almmustuhtton: |
Oxford University Press
2016
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