Detecting and modelling the magnetic field of the<i>β</i> Cephei star V 2052 Ophiuchi

Abstract

Aims. Following the indirect detection of a magnetic field in the β Cephei star V 2052 Oph by Neiner and collaborators in 2003 with the Musicos spectropolarimeter, we remeasured the magnetic field of this star to attempt to directly confirm the detection of a magnetic field and study its configuration in greater detail.