WX Ari is a cataclysmic variable star located in the constellation Aries. It is a close binary system where the white dwarf has a strong magnetic field, which prevents the formation of an accretion disk. Instead, material from the donor red dwarf is funneled along magnetic field lines directly onto the magnetic poles of the white dwarf. The system shows significant brightness variations and variable polarization of light, both typical features of polars.

Photometry & Images

Catalogue Gaia
RA 41.900963715°
DEC 10.593739445°
U --
B --
V --
Parallax (mas) 1.77 ± 0.05
Light curve

TESS Data

43 70 71

AAVSO Data

aavsodataimage

References

Rodríguez-Gil P. et al. Long-term photometry of WX Arietis: evidence for eclipses and dips //arXiv preprint astro-ph/9911303. – 1999.