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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, with the location of NGC 2035 and NGC 2032 marked just left of centre. 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. [2] It was discovered by James Dunlop on August 3, 1826. Its apparent ...
A large ring of cold gas that formed from a collision of two galaxies. [3] Magellanic Stream: 600,000 ly (180,000 pc) [4] complex of HVCs: Connects the Large and Small Magellanic clouds; extends across 180° of the sky. Lyman-alpha blob 1: 300,000 ly (92,000 pc) [5] LαB: Largest blob in the LAB Giant Concentration [citation needed] Himiko Gas ...
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 ]
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.
Diameter (ly) Millions of ... Satellite of Milky Way possibly associated with the Large Magellanic Cloud [15] 300 ly [15 ... Small Magellanic Cloud (SMC, NGC 292) SB ...
The Large Magellanic Cloud, for instance, has less dust than the Milky Way and a smaller content of what astronomers call metallic elements - those other than hydrogen and helium.
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 ]