EE Pegasi
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Pegasus |
| Right ascension | 21h 40m 01.88177 s[1] |
| Declination | +09° 11′ 05.1147″[1] |
| Apparent magnitude (V) | 6.98[1] |
| Distance | 89 ly ( pc) |
| Spectral type | A1III |
| Other designations | |
| Database references | |
| SIMBAD | data |
EE Pegasi is an eclipsing binary star system in the constellation Pegasus. The two main components are two main sequence stars of spectral types A3V and F5V, with a third, smaller, star that is an orange or red dwarf orbiting the main pair every four years.[2]
References
- 1 2 3 SIMBAD, EE Peg (accessed 14 February 2014)
- ↑ Lacy, Claud H.; Popper, Daniel M. (1984). "Absolute dimensions and masses of eclipsing binaries. IV - EE Pegasi is a triple star". Astrophysical Journal. 281 (1): 268–75. Bibcode:1984ApJ...281..268L. doi:10.1086/162096.
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