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According to A.M. Garcia, NGC 4722 is part of NGC 4699 Group (also known as LGG 307), which contains at least 15 galaxies, including NGC 4699, NGC 4700, NGC 4742, NGC 4781, NGC 4790, NGC 4802, and NGC 4818. [5] The NGC 4699 group is part of the Virgo II cluster, a cluster located at the southern boundary of the Virgo Cluster. [6]
NGC 4727 is a large barred spiral galaxy in the constellation of Corvus.Its velocity with respect to the cosmic microwave background for is 7,830 ± 23 km/s, which corresponds to a Hubble distance of 376.7 ± 26.4 Mly (115.49 ± 8.09 Mpc). [1]
Erik Holmberg described multiple galaxies that have since been named after him: Holmberg II is a dwarf irregular galaxy about 9.8 million light-years away in the M81 Group Holmberg IX is a dwarf irregular galaxy and a satellite galaxy of Messier 81.
Size: The average photo frame measures about 10 inches diagonally, roughly the same as an entry-level iPad. I'd consider that the minimum size; anything smaller will make it hard to view photos ...
Seen nearly edge-on, NGC 4216 is one of the largest and brightest spiral galaxies of the Virgo Cluster, with an absolute magnitude that has been estimated to be −22 (i.e.: brighter than the Andromeda Galaxy), [4] and like most spiral galaxies of this cluster shows a deficiency of neutral hydrogen that is concentrated within the galaxy's optical disk and has a low surface density for a galaxy ...
NGC 4725 is an intermediate barred spiral galaxy with a prominent ring structure, [9] located in the northern constellation of Coma Berenices near the north galactic pole. [10] It was discovered by German-born British astronomer William Herschel on April 6, 1785. [11]