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Loss of Mass and Stability of Galaxies in Modified Newtonian DynamicsThe galactic potential and the asymmetric distribution of hypervelocity starsMilky Way potentials in cold dark matter and MOdified Newtonian Dynamics. Is the Large Magellanic Cloud on a bound orbit?Does the galaxy NGC1052–DF2 falsify Milgromian dynamics?
P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
Xufen Wu
@ast
Xufen Wu
@en
Xufen Wu
@es
Xufen Wu
@nl
type
label
Xufen Wu
@ast
Xufen Wu
@en
Xufen Wu
@es
Xufen Wu
@nl
prefLabel
Xufen Wu
@ast
Xufen Wu
@en
Xufen Wu
@es
Xufen Wu
@nl
P106
P31
P496
0000-0002-1378-8082