Gas dynamics in tidal dwarf galaxies: disc formation at z=0
F. Lelli, P.-A. Duc, E. Brinks, F. Bournaud, S. S. McGaugh, U., Lisenfeld, P. M. Weilbacher, M. Boquien, Y. Revaz, J. Braine, B. S., Koribalski, and P.-E. Belles

TL;DR
This study investigates the gas dynamics of tidal dwarf galaxies, revealing they are likely devoid of dark matter and challenging existing theories, by analyzing HI data and disc models across multiple systems.
Contribution
It provides the first detailed analysis of gas dynamics in bona-fide TDGs, confirming their baryonic mass dominance and their deviation from the baryonic Tully-Fisher relation.
Findings
HI discs are consistent with rotation but may not be in full dynamical equilibrium.
Dynamical masses match baryonic masses, indicating lack of dark matter.
TDGs deviate from the baryonic Tully-Fisher relation.
Abstract
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, since they can form only from dissipative material ejected from the discs of the progenitor galaxies. We investigate the gas dynamics in a sample of six bona-fide TDGs around three interacting and post-interacting systems: NGC 4694, NGC 5291, and NGC 7252 ("Atoms for Peace"). For NGC 4694 and NGC 5291 we analyse existing HI data from the Very Large Array (VLA), while for NGC 7252 we present new HI observations from the Jansky VLA together with long-slit and integral-field optical spectroscopy. For all six TDGs, the HI emission can be described by rotating disc models. These HI discs, however, have undergone less than a full rotation since the time of the interaction/merger event, raising the question of…
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