MASTER OT J190519.41+301524.4
An Eclipsing Cataclysmic Variable Star
MASTER OT J190519.41+301524.4 is an eclipsing VY Scl–type cataclysmic variable star in the constellation Vulpecula. In this close binary system, a white dwarf accretes material from a donor star via an accretion disk. The system exhibits deep V-shaped eclipses of about 2 magnitudes and has an orbital period of approximately 3.11 hours. It was discovered in 2014 and thoroughly characterized in 2016.
Photometry & Images
| Catalogue | Gaia |
| RA | 286.330855634° |
| DEC | 30.256800943° |
| U | -- |
| B | -- |
| V | -- |
| Parallax (mas) | 0.87 ± 0.03 |
TESS Data
