NGC 5927 explained

NGC 5927
Class:VIII
Epoch:J2000
Constellation:Lupus
Ra:[1]
Dist Ly:25.1 kly
(7.7 kpc)
Appmag V:8.86
Radius Arcminsec:6.0' x 6.0'[2]
Metal Fe:-0.49[3]
Names:GCl 35, GCRV 5278 E, VDBH 173

NGC 5927 is a globular cluster in the constellation Lupus. NGC 5927 has a diameter of about 12 arcminutes and an apparent magnitude of +8.86. Its Shapley–Sawyer Concentration Class is VIII,[2] and it contains stars of magnitude 15 and dimmer.

The globular cluster was discovered by the astronomer James Dunlop in 1826 and was also observed in 1834 by John Herschel.[4]

NGC 5927 is relatively metal-rich for a globular cluster, and may have multiple generations of stars.

External links

Notes and References

  1. NGC 5927. 8 January 2017.
  2. Web site: NGC 5927. 8 January 2016.
  3. Web site: A Galactic Globular Clusters Database: NGC 5927. 8 January 2017.
  4. Web site: New General Catalog Objects: NGC 5900 - 5949. 2021-03-11. cseligman.com.