NGC 3746 | |
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![]() NGC 3746 (center) with NGC 3745 (left), imaged by Kitt Peak National Observatory | |
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 37m 43.6312s [1] |
Declination | +22° 00′ 35.153″ [1] |
Redshift | 0.030072 [1] |
Heliocentric radial velocity | 9,015 ± 2 km/s [1] |
Distance | 449.2 ± 31.5 Mly (137.72 ± 9.65 Mpc) [1] |
Group or cluster | Copeland Septet |
Apparent magnitude (V) | 15.01 [1] |
Characteristics | |
Type | SB(r)b [1] |
Size | ~44,400 ly (13.62 kpc) (estimated) [1] |
Apparent size (V) | 1.1′ × 0.5′ [1] |
Other designations | |
Copeland Septet NED02, HCG 057B, 2MASS J11374363+2200353, 2MASX J11374364+2200349, UGC 6597, LEDA 35997, MCG +04-28-005, PGC 35997, CGCG 127-006, SDSS J113743.62+220035.3 [1] |
NGC 3746 is a large barred spiral galaxy with a ring structure [2] located in the Leo constellation. [3] It is located 449 million light-years from the Solar System and has an approximate diameter of 45,000 light-years. [1] NGC 3746 was discovered by Ralph Copeland on 9 February 1874 with subsequent observations made by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer. [4]
The luminosity class of NGC 3746 is II and it has a broad H II region with a recessed core (RET). [1]
NGC 3746 is a member of the Copeland Septet which comprises 7 galaxies discovered by Copeland in 1874. [5] The other 6 members are NGC 3745, NGC 3748, NGC 3750, NGC 3751, NGC 3753, and NGC 3754. Together, they are known as Hickson 57 and Arp 320. [6]
Two supernovae have been discovered in NGC 3746: