  The "Binarity and Magnetic Interactions in various classes of stars"
(BinaMIcS) project is based on two large programs of spectropolarimetric
observations with ESPaDOnS at CFHT and Narval at TBL. Three samples of
spectroscopic binaries with two spectra (SB2) are observed: known cool magnetic
binaries, the few known hot magnetic binaries, and a survey sample of hot
binaries to search for additional hot magnetic binaries. The goal of BinaMIcS
is to understand the complex interplay between stellar magnetism and binarity.
To this aim, we will characterise and model the magnetic fields, magnetospheric
structure and coupling of both components of hot and cool close binary systems
over a significant range of evolutionary stages, to confront current theories
and trigger new ones. First results already provided interesting clues, e.g.
about the origin of magnetism in hot stars.
