Many notable nebulae in this Northern section of the Large Megalanic Cloud:

NGC 2035 (also known as ESO 56-EN161 and the Dragon's Head Nebula) is an emission nebula and a H II region in the Dorado constellation and part of the Large Magellanic Cloud. It was discovered by James Dunlop on August 3, 1826. Its apparent size is 3.0.

NGC 2035 is part of a complex of nebulae and stars, including NGC 2029, NGC 2032 and NGC 2040, found north of the main bar of the LMC. It consists of large bright gas clouds which are separated by dark dust clouds. NGC 2029, NGC 2032 and NGC 2035 are star-forming regions, while NGC 2040 is a supernova remnant which contains an open cluster.

NGC 2014 is a red emission nebula surrounding an open cluster of stars in the Large Magellanic Cloud, at a distance of about 163,000 light-years.

The nebula was discovered on 3 August 1826 by Scottish astronomer James Dunlop. Together with NGC 2020 it makes up what is called the Cosmic Reef.

NGC 2030 is an Elliptical Galaxy located in the constellation of Dorado in the southern hemisphere.

NGC 2029 (also known as ESO 56-EN156 or the Dragon's Head Nebula) is an emission nebula in the Dorado constellation and is part of the Large Magellanic Cloud. It is part of a complex of nebulae and stars, including NGC 2032, NGC 2035 and NGC 2040. It was discovered by James Dunlop on the 27 September 1826. Its apparent magnitude is 12.29, and its size is 2.25 arc minutes.

The coordinates for NGC 2029 and NGC 2030 were reversed between Herschel's original Catalogue of Nebulae and Clusters of Stars and the New General Catalogue. NGC 2030, originally GC 2029, is an isolated nebula with an embedded star cluster, about 1.5 degrees north of NGC 2029.

NGC 2004 (also known as ESO 86-SC4) is an open cluster of stars in the southern constellation of Dorado. It was discovered by Scottish astronomer James Dunlop on September 24, 1826. This is a young, massive cluster with an age of about 20 million years and 23,000 times the mass of the Sun. It has a core radius of 2.85 ± 0.46 pc (9.3 ± 1.5 ly). NGC 2004 is a member of the Large Magellanic Cloud, which is a satellite galaxy of the Milky Way.