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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 and its neighbour and relative, the Small Magellanic Cloud, are conspicuous objects in the southern hemisphere, looking like separated pieces of the Milky Way to the naked eye. Roughly 21° apart in the night sky, the true distance between them is roughly 75,000 light-years.
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 ]
NGC 2004 is a member of the Large Magellanic Cloud, [4] which is a satellite galaxy of the Milky Way. References External links. Media related to NGC 2004 at ...
N119's location within the Large Magellanic Cloud. With a right ascension of 5 h 18 m 45 s and a declination of −69° 14′ 03″, [1] this nebula may be found in the constellation of Dorado about 160 kly (50 kpc) away. Its apparent size is roughly 9′ 14″ × 12′ 15″.
The largest of these is the Large Magellanic Cloud with a diameter of 32,200 light-years. [278] It has a close companion, the Small Magellanic Cloud . The Magellanic Stream is a stream of neutral hydrogen gas extending from these two small galaxies across 100° of the sky.
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In photographs, the cluster spans an apparent size of 3.50 arc minutes. [1] The core radius has an angular size of 10.7 ± 0.4 arc seconds, [5] while the half-light radius is 24.3 arc seconds. [4] There are a total of 49 known and one candidate RR Lyrae variable stars in the cluster, as of 2011. Eight are RRd, or double-mode RR Lyrae variables.