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...
Main Authors: | Janz, J, Cappellari, M, Romanowsky, A, Ciotti, L, Alabi, A, Forbes, D |
---|---|
Format: | Journal article |
Published: |
Oxford University Press
2016
|
Similar Items
-
Implications for the origin of early-type dwarf galaxies – the discovery of rotation in isolated, low-mass early-type galaxies
by: Janz, J, et al.
Published: (2017) -
Small scatter and nearly isothermal mass profiles to four half-light radii from two-dimensional stellar dynamics of early-type galaxies
by: Cappellari, M, et al.
Published: (2015) -
A statistical investigation of the mass discrepancy–acceleration relation
by: Desmond, H
Published: (2016) -
Galaxy masses
by: Courteau, S, et al.
Published: (2014) -
Star wars : the making of Episode I :the phantom menace /
by: Bouzereau, Laurent, author, et al.
Published: (1999)