52 Persei
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Perseus |
| Right ascension | 04h 14m 53.32048s[1] |
| Declination | +40° 29′ 01.2303″[1] |
| Apparent magnitude (V) | 4.68[2] |
| Spectral type | G5II + A2V[3] |
| Other designations | |
| Database references | |
| SIMBAD | data |
52 Persei (52 Per) is a spectroscopic binary star in the constellation Perseus. Its apparent magnitude is 4.68.
References
- ^ a b Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- ^ Parsons, Sidney B. (2004). "New and Confirmed Triple Systems with Luminous Cool Primaries and Hot Companions". The Astronomical Journal. 127 (5): 2915. Bibcode:2004AJ....127.2915P. doi:10.1086/383546.
- ^ Markowitz, Allan Henry (1969). "A Study of Stars Exhibiting Composite Spectra". Bibcode:1969PhDT.........5M.
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