52 Persei

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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
52 Persei, HR 1306, HIP 19811, HD 26674, BD+40°912
Database references
SIMBAD data

52 Persei (52 Per) is a spectroscopic binary star in the constellation Perseus. Its apparent magnitude is 4.68.

References[edit]

  1. ^ a b Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653. Bibcode:2007A&A...474..653V. arXiv:0708.1752Freely accessible. doi:10.1051/0004-6361:20078357. 
  2. ^ 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. 
  3. ^ Markowitz, Allan Henry (1969). "A Study of Stars Exhibiting Composite Spectra". Bibcode:1969PhDT.........5M.