RW Tri

RW Trianguli (RW Tri) is a cataclysmic variable star in the constellation Triangulum. It is a binary system consisting of a white dwarf and a red dwarf, between which a continuous mass transfer takes place. RW Tri is a classic example of a nova-like variable star with an accretion disk.

Photometry & Images

Catalogue	Gaia
RA	36.400768695°
DEC	28.097391313°
U	--
B	--
V	--
Parallax (mas)	3.27 ± 0.02

Light curve

fig.2

TESS Data

sectors18

sectors58

sectors85

AAVSO Data

aavsodataimage

Spectroscopy

Spectroscopy Image

References

1. Subebekova G. et al. Structure of accretion flows in the nova-like cataclysmic variable RW Tri //Monthly Notices of the Royal Astronomical Society. – 2020. – Т. 497. – №. 2. – С. 1475-1487.

2. Smak J. RW Tri-its Negative Superhumps and System Parameters //arXiv preprint arXiv:1902.07502. – 2019.

3. Noebauer U. M. et al. The geometry and ionization structure of the wind in the eclipsing nova-like variables RW Tri and UX UMa //The Astrophysical Journal. – 2010. – Т. 719. – №. 2. – С. 1932.

4. Groot P. J., Rutten R. G. M., van Paradijs J. A spectrophotometric study of RW Trianguli //Astronomy & Astrophysics. – 2004. – Т. 417. – №. 1. – С. 283-291.