| NGC 6145 | |
|---|---|
NGC 6145 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Hercules |
| Right ascension | 16h 25m 02.3795s |
| Declination | +40° 56′ 47.926″ |
| Redshift | 0.028671±0.0000105 |
| Heliocentric radial velocity | 8,595±3 km/s |
| Distance | 414.8 ± 29.0 Mly (127.17 ± 8.90 Mpc) |
| Group or cluster | Abell 2199 |
| Apparent magnitude (V) | 14.5g |
| Characteristics | |
| Type | Sb |
| Size | ~149,000 ly (45.68 kpc) (estimated) |
| Apparent size (V) | 0.98′ × 0.5′ |
| Other designations | |
| HOLM 747A, 2MASX J16250238+4056478, MCG +07-34-021, PGC 58074, CGCG 224-017 | |
NGC 6145 is a spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 8,622±4 km/s, which corresponds to a Hubble distance of 414.8 ± 29.0 Mly (127.17 ± 8.90 Mpc). Additionally, one non-redshift measurement gives a farther distance of 460 Mly (140 Mpc). It was discovered by British astronomer John Herschel on 12 May 1828.
NGC 6145 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
NGC 6145 and NGC 6147 are listed together as Holm 747 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937. NGC 6145 is also part of the galaxy cluster known as Abell 2199.
One supernova has been observed in NGC 6145: