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The small scatter of the baryonic Tully-Fisher relation
Federico Lelli, Stacy S. McGaugh, James M. Schombert
In a LCDM cosmology, the baryonic Tully-Fisher relation (BTFR) is expected to show significant intrinsic scatter resulting from the mass-concentration relation of dark matter halos…
The mass discrepancy acceleration relation in a CDM context
Arianna Di Cintio, Federico Lelli
The mass discrepancy acceleration relation (MDAR) describes the coupling between baryons and dark matter (DM) in galaxies: the ratio of total-to-baryonic mass at a given radius ant…
Tidal Dwarf Galaxies: Disc Formation at z=0
Federico Lelli, Pierre-Alain Duc, Elias Brinks +1
Collisional debris around interacting and post-interacting galaxies often display condensations of gas and young stars that can potentially form gravitationally bound objects: Tida…
Gas dynamics in tidal dwarf galaxies: disc formation at z=0
F. Lelli, P. -A. Duc, E. Brinks +9
Tidal dwarf galaxies (TDGs) are recycled objects that form within the collisional debris of interacting/merging galaxies. They are expected to be devoid of non-baryonic dark matter…