NGC 1935 (also known as ESO 56-EN110 and IC 2126) is an emission nebula which is part of the larger LMC-N44 nebula in the Dorado constellation. NGC 1935 is also located 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 1935, then was observed by Williamina Fleming in 1901 and later added to the Index Catalogue as IC 2126.

600/800mm - 24" (4/7/08 - Magellan Observatory, Australia): this emission glow forms a pair NGC 1936 just southeast in a very striking field of clusters and HII patches (part of stellar association LH 47). At 200x and UHC filter it appeared as a very bright, round glow of uniform high surface brightness. The size is slightly smaller than NGC 1936, perhaps 45"-50" in diameter. Good response to the UHC filter. Nebulosity (BSDL 1363) also extends off to the NW of NGC 1935 and a locally brighter patch (NGC 1934) involves a couple of brighter stars.