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Listed below are galaxies with diameters greater than 700,000 light-years. This list uses the mean cosmological parameters of the Lambda-CDM model based on results from the 2015 Planck collaboration, where H 0 = 67.74 km/s/Mpc, Ω Λ = 0.6911, and Ω m = 0.3089. [3]
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HD 33579: 471 [125] Large Magellanic Cloud L/T eff: The brightest star in the Large Magellanic Cloud. S Doradus: 100 [128] Large Magellanic Cloud L/T eff: A luminous blue variable in the S Doradus instability strip. HD 37974: 99 [129] Large Magellanic Cloud L/T eff: An unusual blue hypergiant with a large dusty disk. [129] R136a1: 42.7 +1.6 − ...
A dwarf galaxy is a small galaxy composed of about 1000 up to several billion stars, as compared to the Milky Way's 200–400 billion stars. [1] The Large Magellanic Cloud , which closely orbits the Milky Way and contains over 30 billion stars, [ 2 ] is sometimes classified as a dwarf galaxy; others consider it a full-fledged galaxy.
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η Carinae, a luminous blue variable as seen from the Chandra X-ray Observatory HD 168607 is the right star of the pair below the Omega Nebula. The other is the hypergiant HD 168625 . A selection of LBVs and suspected LBVs with nebula, observed with the Spitzer Space Telescope .
A faint blue galaxy (FBG) is an inconspicuous, often small galaxy with low surface luminosity.In addition to being dim, they show a remarkable preponderance of sparsely scattered blue stars, but comparatively few red stars, which in most galaxies are by far the most common.