Double Cluster

Double Cluster
Caldwell 14 - The Double Cluster taken by /u/ItFrightensMe
The Double Cluster, NGC 869 (above) and NGC 884 (below) with north to the left
Observation data (J2000.0 epoch)
Right ascension2h 20m
Declination57° 08
Distance7,460 and 7,640ly[1] (2,290 and 2340pc[1])
Apparent magnitude (V)3.7 and 3.8
Apparent dimensions (V)60
Physical characteristics
Other designationsCaldwell 14
Associations
ConstellationPerseus
See also: Open cluster, List of open clusters

The Double Cluster (also known as Caldwell 14) consists of the open clusters NGC 869 and NGC 884 (often designated h Persei and χ (chi) Persei, respectively), which are close together in the constellation Perseus. Both visible with the naked eye, NGC 869 and NGC 884 lie at a distance of about 7,500 light years in the Perseus Arm of the Milky Way galaxy.[2]

  1. ^ a b Currie, Thayne; Hernandez, Jesus; Irwin, Jonathan; Kenyon, Scott J.; Tokarz, Susan; Balog, Zoltan; Bragg, Ann; Berlind, Perry; Calkins, Mike (2010). "The Stellar Population of h and χ Persei: Cluster properties, membership, and the intrinsic colors and temperatures of stars". The Astrophysical Journal Supplement. 186 (2): 191. arXiv:0911.5514. Bibcode:2010ApJS..186..191C. doi:10.1088/0067-0049/186/2/191. S2CID 16454332.
  2. ^ Keller, Stefan C.; Grebel, Eva K.; Miller, Grant J.; Yoss, Kenneth M. (2001). "UBVI and Hα photometry of the h and χ Persei cluster". The Astronomical Journal. 122 (1): 248. arXiv:astro-ph/0104179. Bibcode:2001AJ....122..248K. doi:10.1086/321139.