NGC 1936 explained

NGC 1936
Type:Emission
Ra:[1]
Appmag V:11.60 [2]
Size V:12.87
Constellation:Dorado
Names:GC 1142, h 2844, Dunlop 175,[3] IC 2127, ESO 056-EN111

NGC 1936 (also known as IC 2127 and ESO 056-EN111) is an emission nebula which is part of the larger LMC-N44 nebula located in the Dorado constellation in the Large Magellanic Cloud. It was discovered by John Herschel in 1834 and added to the Catalogue of Nebulae and Clusters of Stars as NGC 1936. It was later observed by John Dunlop on September 27, 1936, and Williamina Fleming in 1901 and added to the Index Catalogue as IC 2127.[4] Its apparent magnitude is 11.60.

Notes and References

  1. Web site: Bright Nebula NGC 1936. dso-browser. 14 October 2017.
  2. Web site: IC 2127 -- Emission Object. SIMBAD. 14 October 2017.
  3. Web site: NGC 1936. SEDS. 14 October 2017.
  4. Web site: NGC 1936 (= IC 2127, in the Large Magellanic Cloud). cseligman. 14 October 2017.