GS Pav is a cataclysmic variable star located in the constellation Pavo. It is a close binary system in which a normal star transfers mass to a white dwarf, forming an accretion disk. GS Pav shows brightness variations typical of nova-like stars and may exhibit eclipses, making it valuable for studying the system’s structure.
Photometry & Images
| Catalogue | Gaia |
| RA | 302.031905701° |
| DEC | -69.816420886° |
| U | -- |
| B | -- |
| V | -- |
| Parallax (mas) | 1.85 ± 0.03 |
TESS Data
AAVSO Data
