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. Its apparent magnitude is 11.60.

600/800mm - 24" (4/7/08 - Magellan Observatory, Australia): NGC 1936 appeared as a very bright, round glow, ~1' diameter with a very high, uniform surface brightness at 200x using a UHC filter. Situated at the south end of a large cluster and HII complex. Additional fainter nebulosity sweeps to the south and is connected with a fainter (anonymous) patch to the west by 1'. This extension increases the total size to 2' to 2.5'. NGC 1935 lies 2' NW. This number also applies to the cluster (S-L 417) that spreads out the north. Mag 8.5 HD 35665 lies 7' W.