| Abstract: | A review of selected photometric and spectrophotometric properties of magnetic stars is given. It is shown that unreddened B–V of magnetic stars around B9 type can be transformed to log Te using the calibration for normal stars and no systematic errors are introduced. Mechanisms of light variability are discussed. It is concluded that different mechanisms must be operating in different stars. Recently obtained photometric observations of short-period variability by KURTZ and Hβ variability by MADEJ et al. are discussed. An information about internal structure and the atmospheric structure of these stars can be derived from these observations. |
