A Study of the Photometric Variability of the Peculiar Magnetic White Dwarf WD 1953-011
We present and interpret simultaneous new photometric and spectroscopic observations of the peculiar magnetic white dwarf WD 1953-011. The flux in the V-band filter and intensity of the Balmer spectral lines demonstrate variability with the rotation period of about 1.45 days. According to previous studies, this variability can be explained by the
Valyavin, G. et al.
Fecha de publicación:
6
2011