PAPITTO, ALESSANDROALESSANDROPAPITTODE MARTINO, DomitillaDomitillaDE MARTINO2023-01-092023-01-092022978-3-030-85197-20067-0057http://hdl.handle.net/20.500.12386/32845Millisecond pulsars in tight binaries have recently challenged our understanding of physical processes governing the evolution of binaries and the interaction between astrophysical plasma and electromagnetic fields. Transitional systems that showed changes from rotation-powered to accretion-powered states and vice versa have bridged the populations of radio and accreting millisecond pulsars, eventually demonstrating the tight evolutionary link envisaged by the recycling scenario. A decade of discoveries and theoretical efforts have just grasped the complex phenomenology of transitional millisecond pulsars from the radio to the gamma-ray bands. This chapter summarizes the main properties of the three transitional millisecond pulsars discovered so far, as well as of candidates and related systems, discussing the various models proposed to cope with their multifaceted behaviour.STAMPAenBook part10.1007/978-3-030-85198-9_6https://link.springer.com/chapter/10.1007/978-3-030-85198-9_6https://arxiv.org/pdf/2010.09060.pdf2022ASSL..465..157PFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering