Variations of the Ap star HD 208217 *
Received 25 July 1996 / Accepted 12 September 1996
We present a new determination of the rotation period of the Ap star HD 208217 based on photometric and magnetic measurements. The variations of this star are remarkable by the strong anharmonicity of its lightcurves in all colours as well as by the double wave of its mean magnetic field modulus variations.
Key words: stars: chemically peculiar stars: individual: HD 208217 stars: rotation
© European Southern Observatory (ESO) 1997
Online publication: June 30, 1998