NGC 3748 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 37m 49.065s |
Declination | +22d 01m 34.14s |
Redshift | 0.029407 |
Heliocentric radial velocity | 8,816 km/s |
Distance | 440 Mly (135 Mpc) |
Group or cluster | Copeland Septet |
Apparent magnitude (V) | 14.8 |
Characteristics | |
Type | SB0?, S0, RET |
Size | 148,000 ly |
Other designations | |
PGC 36007, CGCG 127-007, MCG +04-28-007, Copeland Septet NED03, 2MASX J11374903+2201340, NSA 139941, HCG 057E, SDSS J113749.06+2201134.1, WBL 343-002, UZC J113749.1+220134, SSTSL2 J113749.06+220134.2, 2XMM J113749.0+220133, LEDA 36007 |
NGC 3748 is a lenticular galaxy with a bar[1] located in the Leo constellation.[2][3] It is located 440 million light-years away from the Solar System[4] and was discovered by Ralph Copeland on April 5, 1874, but also observed by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.[5]
Like NGC 3746, NGC 3748 also has a recessed core (RET).[4] It is described as, "moderately bright, fairly small, slightly elongated NW-SE, 0.4'x0.3' with a small bright core".[6]