No document available.
Abstract :
[en] In our previous low-resolution spectropolarimetric observations with the Very Large Telescope (VLT), three slowly pulsating B-type (SPB) stars, HD 74195, HD 74560, and HD 85953, showed the presence of a weak magnetic field. The results of our new measurements, using high-resolution spectropolarimetric observations, formally showed significant detections above the 3σ level in the SPB stars HD 74195 and HD 85953.