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NGC 2566 is a barred spiral galaxy in the constellation of Puppis.Its velocity with respect to the cosmic microwave background is 1898 ± 19 km/s, which corresponds to a Hubble distance of 91.3 ± 6.5 Mly (28.00 ± 1.98 Mpc). [1]
The larger spiral, NGC 2207, is classified as an intermediate spiral galaxy exhibiting a weak inner ring structure around the central bar. The smaller companion spiral, IC 2163, is classified as a barred spiral galaxy that also exhibits a weak inner ring and an elongated spiral arm that is likely being stretched by tidal forces with the larger ...
NASA’s Hubble Space Telescope recently captured a breathtaking image of the spiral galaxy NGC 2566. Astronomers use detailed Hubble images to study star clusters and active star-forming regions.
NGC 3190 is a spiral galaxy with tightly wound arms and lying in the constellation Leo.It was discovered by William Herschel in 1784. NGC 3190 is member of Hickson 44 galaxy group, estimated at around 80 million light years away, [2] and consisting of four galaxies in a tight group - NGC 3193 is fairly featureless, NGC 3187 is a dim but striking spiral galaxy and NGC 3185 has a barred spiral ...
NGC 1300 is a barred spiral galaxy located about 65 million light-years away in the constellation Eridanus.The galaxy is about 110,000 light-years across. It is a member of the Eridanus Cluster, a cluster of 200 galaxies, [3] [4] [5] in a subgroup of 2-4 galaxies in the cluster known as the NGC 1300 Group.
NGC 6872 is interacting with the lenticular galaxy IC 4970, which is less than one twelfth as large. [ 2 ] [ 3 ] The galaxy has two elongated arms with a diameter based on ultraviolet light of over 522,000 light-years (160,000 pc ), and a D 25.5 isophotal diameter of over 717,000 light-years (220,000 pc ), making it the largest known spiral ...
UGC 3478 is a spiral galaxy, located in the constellation of Camelopardalis. [ 3 ] [ 4 ] Is is located at 128 million light-years from Earth. [ 5 ] It features a growing supermassive black hole (AGN) at its center.