ASASSN-13cx is a cataclysmic variable star of the dwarf nova type, located in the constellation Andromeda. It was discovered in 2013 by the ASAS-SN survey as a transient object that brightened by approximately 4 magnitudes. The system consists of a white dwarf accreting matter from a donor star via an accretion disk. Instabilities in the disk cause recurrent outbursts of brightness, a hallmark of dwarf nova behavior.

Photometry & Images

Catalogue Gaia
RA 0.593266990°
DEC 42.703667149°
U --
B --
V --
Parallax (mas) 2.49 ± 0.13
Light curve

TESS Data

sectors17 sectors84

AAVSO Data

aavsodataimage

References

Kato T. et al. Survey of period variations of superhumps in SU UMa-type dwarf novae. VII. The seventh year (2014–2015) //Publications of the Astronomical Society of Japan. – 2015. – Т. 67. – №. 6. – С. 105.