Observatoire Astronomique de Strasbourg - OAS - UMR7550

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Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
Current data on the globular cluster Palomar 14 are consistent with MOND
Dark matter–baryon scaling relations from Einasto halo fits to SPARC galaxy rotation curves
Detection of a radial velocity gradient in the extended local disc with RAVE
Discussing the first velocity dispersion profile of an ultra-diffuse galaxy in MOND
Distribution functions for Galactic disc stellar populations in the presence of non-axisymmetric perturbations
Distribution functions for resonantly trapped orbits in our Galaxy
Distribution functions for resonantly trapped orbits in the Galactic disc
Dynamical measurement of the stellar surface density of face-on galaxies
Early- and late-stage mergers among main sequence and starburst galaxies at 0.2 ≤ z ≤ 2
The effects of bar–spiral coupling on stellar kinematics in the Galaxy
Electrodynamics and Radiation from Rotating Neutron Star Magnetospheres
Emergence of the mass discrepancy-acceleration relation from dark matter-baryon interactions
Emergent gravity in galaxies and in the Solar System
Equilibrium configurations of 11 eV sterile neutrinos in MONDian galaxy clusters
The escape speed curve of the Galaxy obtained from Gaia DR2 implies a heavy Milky Way
Evolution of galactic discs: multiple patterns, radial migration, and disc outskirts
Exploring the reality of density substructures in the Palomar 5 stellar stream
Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

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