NGC 1761

NGC 1761 is an open cluster in the Dorado constellation in the Large Magellanic Cloud. It encompasses a group of about 50 massive hot young stars. These stars are among the largest stars known anywhere in the Universe and appear as bright blue-white in colour. The stars in turn have given birth to new stars within dark globules. NGC 1761 is particularly noteworthy for its intense ultraviolet radiation, which has eroded a large hole in the surrounding nebular material. It is similar in structure to the more famous Rosette Nebula.
It is part of a large region of stars called LMC-N11 which was discovered with a 23-cm telescope by the astronomer James Dunlop in 1826 and was also observed by John Herschel in 1835.