Speaker
Prof.
Fabio Iocco
(Università di Napoli "Federico II")
Description
The (in)famous method of "Rotation Curves" has informed us for decades about the mass structure of disk galaxies. Does modern technology allow us to hope for a more informative method? I will describe some recent work that hints towards a positive answer.
https://arxiv.org/abs/2111.08725
Primary author
Prof.
Fabio Iocco
(Università di Napoli "Federico II")
