Jump to content

NGC 1856

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by InternetArchiveBot (talk | contribs) at 03:06, 12 April 2020 (Rescuing 1 sources and tagging 0 as dead.) #IABot (v2.0). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

NGC 1856
Hubble Space Telescope photograph of NGC 1856
Observation data (J2000.0 epoch)
ConstellationDorado
Right ascension05h 09m 29.4s[1]
Declination−69° 07′ 39″[1]
Apparent magnitude (V)10.1[2]
Physical characteristics
See also: Globular cluster, List of globular clusters

NGC 1856 is a young, massive star cluster similar to a "blue globular cluster"[3] in the Magellanic Clouds in the constellation Dorado. Its age is estimated to be 80 million years.[3] The object was discovered in 1826 by James Dunlop with a 9-inch reflecting telescope.[4]

Sources

  1. ^ a b NASA/IPAC Extragalactic Database
  2. ^ "NGC 1856". SIMBAD. Centre de données astronomiques de Strasbourg.
  3. ^ a b Hodge, P. W.; Lee, S.-O.: LMC blue globular clusters containing Cepheids. I. NGC 1856; ApJ 276, S. 509-518 (1984)
  4. ^ "NGC/IC Project". Archived from the original on 2012-12-18. Retrieved 2020-04-12.
  • Media related to NGC 1856 at Wikimedia Commons