NGC 6087 explained

NGC 6087
Type:Open Cluster
Epoch:J2000
Ra:[1]
Dist Ly:~3500LY
Dist Pc:~1000pc
Appmag V:5.4
Size V:12
Constellation:Norma
Names:S Normae Cluster, Caldwell 89, Cr 300

NGC 6087 (also known as Caldwell 89 or the S Normae Cluster) is an open cluster of 40 or more[2] stars centered on the Cepheid variable S Normae in the constellation Norma. At a distance of about 3500 ly and covering a field of almost one quarter of a degree, the stars range from seventh- to eleventh-magnitude, the brightest being 6.5 magnitude S Normae. The aggregate visual magnitude of the cluster is about 5.4.

Spectral analysis of the radial motion of the stars confirm that S Normae is a member of the cluster,[3] and the period/luminosity relationship of Cepheid variables allows the distance to be determined with confidence.

Notes and References

  1. NGC 6087 . 2007-04-18.
  2. [Robert Burnham, Jr.|Burnham]
  3. A. U. Landolt. 1964. The Galactic Cluster NGC 6087. Astrophysical Journal Supplement. 8. 329–351. 4 April 2013. 1964ApJS....8..329L . 10.1086/190092 . free.