Search results
Results from the WOW.Com Content Network
The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. [7] At a distance of around 50 kiloparsecs (163,000 light-years), [2] [8] [9] [10] the LMC is the second- or third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal (c. 16 kiloparsecs (52,000 light-years) away) and the possible dwarf irregular galaxy called the Canis Major Overdensity.
The Large Magellanic Cloud was the host galaxy to a supernova , the brightest observed in over four centuries. Measurements with the Hubble Space Telescope, announced in 2006, suggest the Magellanic Clouds may be moving too fast to be long term companions of the Milky Way . [ 34 ]
The N 70 Nebula, in the Large Magellanic Cloud has a shell structure and is really a bubble in space. It is a "Super Bubble". Barnard's Loop: 300 ly (92 pc) [47] [48] H II region: Supernova over the last 4 million years probably carved cavities in gas clouds forming the semi circle shape of Barnard’s loop. Sh2-54: 252 ly (77 pc) [49] [50] H ...
NGC 1974 (also known as NGC 1991 and ESO 85-SC89) is an open cluster associated with an emission nebula which is located in the Dorado constellation which is part of the Large Magellanic Cloud. It was discovered by James Dunlop on November 6, 1826, and later observed by John Herschel on January 2, 1837, subsequently cataloged as NGC 1991. [ 4 ]
N119 (formally known as LHA 120-N 119) is a spiral-shaped H II region in the Large Magellanic Cloud. Its dimensions are large, at 131 x 175 pc (430 × 570 ly). [2] It contains several luminous stars including S Doradus, LH41-1042, and LMC195-1. Its peculiar S-shaped structure is difficult to explain with classical models.
It belongs to the Large Magellanic Cloud, a satellite galaxy to the Milky Way, which is at a distance of 168,000 light years. [1] NGC 2080 was discovered by John Frederick William Herschel in 1834. [2] The Ghost Head Nebula has a diameter of 50 light-years [3] and is named for the two distinct white patches it possesses, called the "eyes of the ...
NGC 2027 (also known as ESO 86-SC13) is a 12th magnitude open cluster located in the Dorado constellation which is also part of the Large Magellanic Cloud and was discovered by James Dunlop on November 6, 1826. [2] Its apparent diameter is 0.7 arcminutes. [2]
NGC 1955 (also known as ESO 56-SC121) is an open cluster associated with an emission nebula located in the Dorado constellation. This nebula is part of the H II region [5] which is part of the Large Magellanic Cloud and was discovered by James Dunlop on August 3, 1826. [3]