Measuring surface magnetic fields of red supergiant stars

Abstract

Context.Red supergiant (RSG) stars are very massive cool evolved stars. Recently, a weak magnetic field was measured at the surface ofαOri and this is so far the only M-type supergiant for which a direct detection of a surface magnetic field has been reported.Aims.By extending the search for surface magnetic field in a sample of late-type supergiants, we want to determine whether the surface magnetic field detected onαOri is a common feature among the M-type supergiants.Methods.With the spectropolarimeter Narval at TélescopeBernard-Lyotwe undertook a search for surface magnetic fields in a sample of cool supergiant stars, and we analysed circular polarisation spectra using the least-squares deconvolution technique.Results.We detect weak Zeeman signatures of stellar origin in the targets CE Tau,α1Her andμCep. For the latter star, we also show that cross-talk from the strong linear polarisation signals detected on this star must be taken into account. For CE Tau andμCep, the longitudinal component of the detected surface fields is at the Gauss-level, such as inαOri. We measured a longitudinal field almost an order of magnitude stronger forα1Her. We also report variability of the longitudinal magnetic field of CE Tau andα1Her, with changes in good agreement with the typical atmospheric dynamics time-scales. We also report a non-detection of magnetic field at the surface of the yellow supergiant starρCas.Conclusions.The two RSG stars of our sample, CE Tau andμCep, display magnetic fields very similar to that ofαOri. The non-detection of a magnetic field on the post-RSG starρCas suggests that the magnetic field disappears, or at least becomes undetectable with present methods, at later evolutionary stages. Our analysis ofα1Her supports the proposed reclassification of the star as an M-type asymptotic giant branch star.