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The Sombrero Galaxy (also known as Messier Object 104, M104 [4] or NGC 4594) is a peculiar galaxy of unclear classification [5] in the constellation borders of Virgo and Corvus, being about 9.55 megaparsecs (31.1 million light-years) [2] from the Milky Way galaxy.
NASA's James Webb Space Telescope has returned incredible new photos of the Sombrero galaxy, offering a new look at the region. The Sombrero galaxy, named for its resemblance to the Mexican hat ...
IC 1101 is a class S0 supergiant lenticular galaxy at the center of the Abell 2029 galaxy cluster.It has an isophotal diameter at about 123.65 to 169.61 kiloparsecs (400,000 to 550,000 light-years).
NGC 5746 is located at a distance of 99 million light years [7] and is seen nearly edge-on, bearing a strong resemblance with the galaxy NGC 4565, that is also seen nearly edge-on. Galaxy NGC 5746, by HST. As with the former, it has a box-shaped bulge that is actually a bar seen from one side [7] and a currently modest star formation activity. [8]
But the Sombrero galaxy is quiet in terms of star formation compared with other galaxies such as Messier 82. Ten times as many stars are born in the latter galaxy than the estimated 100 billion ...
Spitzer's full view shows the disk is warped, which is often the result of a gravitational encounter with another galaxy, and clumpy areas spotted in the far edges of the ring indicate young star-forming regions. The Sombrero galaxy is located some 28 million light-years away. Viewed from Earth, it is just six degrees south of its equatorial plane.
A1689-zD1 is a galaxy in the Virgo constellation. It was a candidate for the most distant and therefore earliest-observed galaxy discovered as of February 2008, based on a photometric redshift. [1] [2] If the redshift, z~7.6, [3] is correct, it would explain why the galaxy's faint light reaches us at infrared wavelengths.
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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