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...
المؤلفون الرئيسيون: | Janz, J, Cappellari, M, Romanowsky, A, Ciotti, L, Alabi, A, Forbes, D |
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التنسيق: | Journal article |
منشور في: |
Oxford University Press
2016
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مواد مشابهة
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