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 ]
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 ]
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 ...
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.
Its apparent size is 2.5 arcmin. It is located in the Large Magellanic Cloud. [4] References External links. Media related to NGC 2164 at Wikimedia ...
NCG 5204 is a Magellanic spiral galaxy located about 14.5 million light-years away from Earth [note 1] in the constellation of Ursa Major and is a member of the M101 Group of galaxies. [4] [5] It has a galaxy morphological classification of SA(s)m and is highly irregular, with only the barest indication of any spiral arm structure. [3]
NGC 2002 (also known as ESO 86-SC3) is an open cluster located in the Dorado constellation and is part of the Large Magellanic Cloud. It was discovered by James Dunlop on September 24, 1826. Its apparent magnitude is 10.1, and its size is 2.0 arc minutes. [1] [3] NGC 2002 contains five red supergiants, prominent in deep images of the cluster.