SIMBAD references

We analyzed magnetic-field structures of three three-dipole magnetic stars HD 18078, HD 37776, and HD 149438. The fact that the model and observed phase dependences B_e and B_s for HD 18078 computed with the same parameters of the dipoles agree with each other shows conclusively that global magnetic structures are formed by dipole structures. Magnetic poles show up conspicuously on Mercator maps of the distribution of magnetic field, the field strength there is maximal and equal to B_p = 3577, 10 700, and 275 G in the three stars mentioned above.Dipole modelsmake it possible to analyze magnetic-field structure inside stars.