NGC 249 is an emission nebula in the constellation Tucana. It was discovered on 5 September 1826 by the astronomer James Dunlop. [3]

NGC 249 is a HII Ionized region in the Tucana constellation. NGC 249 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its B magnitude of 13.8, NGC 249 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

NGC 249 is a captivating emission nebula (a cloud of high temperature gas) situated in the Tucana constellation. This astronomical marvel was first observed on September 5, 1826, by the renowned astronomer James Dunlop.

NGC 249 (NGC249) is a emission nebula that has a distance from Earth of light years. It can be found in the constellation of Tucana.

2023年8月23日 · Historical Identification: Per Dreyer, NGC 200 (= GC 104 = WH II 858, 1860 RA 00 32 23, NPD 87 53.0) is "pretty bright, small, very gradually brighter middle".

Gravitational interactions with the MW and the nearby Large Magellanic Cloud (LMC), a larger dwarf galaxy, have sturred this molecular cloud and created centers of star-birth activity within it. A gravitational "tail" of stars and gas can be seen reaching from the SMC to the LMC.

NGC 249 in Small Magellanic Cloud. Inside the Small Magellanic Cloud. Centered on NGC 249 an emission nebula within a large ionized HII region, the Small Magellanic Cloud a dwarf galaxy which is a satellite of the Milky Way hosts numerous nebulae and star clusters that are visible to astrophotographers.

< NGC List NGC 249. NGC 249 is a H II region located in the constellation of Tucana. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 249:

NGC 249. Inside the Small Magellanic Cloud. Centered on NGC 249 an emission nebula within a large ionized HII region, the Small Magellanic Cloud a dwarf galaxy which is a satellite of the Milky Way hosts numerous nebulae and star clusters that are visible to astrophotographers.

NGC 249 is an emission nebula in the constellation Tucana. It was discovered on 5 September 1826 by the astronomer James Dunlop.