NGC 2748 | |
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![]() NGC 2748 imaged by the Hubble Space Telescope | |
Observation data (J2000.0 epoch) | |
Constellation | Camelopardalis |
Right ascension | 09h 13m 43.037s [1] |
Declination | +76° 28′ 31.23″ [1] |
Redshift | 0.004930 [2] |
Heliocentric radial velocity | 1,473 km/s [3] |
Distance | 61.3 Mly (18.79 Mpc) [3] |
Apparent magnitude (V) | 11.7 [4] |
Characteristics | |
Type | SAbc [5] |
Apparent size (V) | 2.250 × 0.720 arcmin [2] |
Other designations | |
UGC 4825, MCG +13-07-019, PGC 26018 [2] |
NGC 2748 is a spiral galaxy in the northern circumpolar constellation of Camelopardalis, [6] located at a distance of 61.3 megalight-years from the Milky Way. [3] It was discovered September 2, 1828 by John Herschel. [6] The morphological classification of SAbc [5] indicates this is an unbarred spiral with moderate to loosely-wound spiral arms. It is a disk-like peculiar galaxy with a stellar shell that is rotating about the main galactic axis. This shell was most likely formed through the capture and disruption of a dwarf companion. [7] The galactic nucleus likely contains a supermassive black hole with a mass of 4.4+3.5
−3.6×107 M☉ , or 44 million times the mass of the Sun. [5]
Three supernovae and one luminous red nova have been observed in NGC 2748.