The mass discrepancy acceleration relation in early-type galaxies: extended mass profiles and the phantom menace to MOND

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...

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Dettagli Bibliografici
Autori principali:	Janz, J, Cappellari, M, Romanowsky, A, Ciotti, L, Alabi, A, Forbes, D
Natura:	Journal article
Pubblicazione:	Oxford University Press 2016

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