VizieR Online Data Catalog: MiMeS magnetic analysis of O-type stars (Grunhut+, 2017)

As described by Paper I (Wade et al., 2016, Cat. J/MNRAS/456/2), high-resolution circular polarization (Stokes V) spectra of 110 Wolf-Rayet (WR) and O-type targets were collected in the context of the MiMeS project. Of these targets, three magnetic stars (theta¹ Ori C, Donati et al., 2002MNRAS.333...55D; zeta Ori A, Bouret et al., 2008MNRAS.389...75B; and HD 191612, Donati et al., 2006MNRAS.365L...6D) were previously known or highly suspected to host a magnetic field and were observed as part of the targeted component (TC). The 11 WR stars were previously discussed by de la Chevrotiere et al. (2013ApJ...764..171D) and de la Chevrotiere et al. (2014ApJ...781...73D) and are not further discussed here with the exception of HD 190918, which also contains a spectroscopic O-star companion that is included in this study. In this paper, we focus on the 97 survey component (SC) systems that host an O-type star.

A total of 879 Stokes V observations of these 97 targets were obtained with the Echelle SpectroPolarimetric Device for the Observations of Stars (ESPaDOnS), Narval, and HARPSpol echelle spectropolarimeters.

(3 data files).