Magnetic Field Structures of the Stars HD 94660, HD 75049, and HD 154708

Based on published data, we have constructed models for the magnetic structures of three stars with a relatively strong magnetic field. They all have a dipolar structure and do not differ in their properties from the bulk of the magnetic stars. However, they, as well as some other objects with a strong magnetic field, do not obey the direct dependence of the rotation period on the stellar magnetic field strength that is expected from the hypothesis about the loss of angular momentum by its transfer to the surrounding protostellar clouds through magnetic field lines.