| NGC 4619 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Canes Venatici |
| Right ascension | 12h 41m 44.5498s |
| Declination | +35° 03′ 45.776″ |
| Redshift | 0.023093±0.00000667 |
| Heliocentric radial velocity | 6,923±2 km/s |
| Distance | 331.74 ± 12.34 Mly (101.713 ± 3.783 Mpc) |
| Apparent magnitude (V) | 13.5g |
| Characteristics | |
| Type | SB(r)b pec |
| Size | ~149,200 ly (45.76 kpc) (estimated) |
| Apparent size (V) | 1.25′ × 1.06′ |
| Other designations | |
| IRAS 12393+3520, 2MASX J12414453+3503463, UGC 7856, MCG +06-28-018, PGC 42594, CGCG 188-014 | |
NGC 4619 is a barred spiral galaxy in the constellation of Canes Venatici. Its velocity with respect to the cosmic microwave background is 7,176±18 km/s, which corresponds to a Hubble distance of 345.2 ± 24.2 Mly (105.84 ± 7.41 Mpc). However, 15 non-redshift measurements give a closer mean distance of 331.74 ± 12.34 Mly (101.713 ± 3.783 Mpc). It was discovered by German-British astronomer William Herschel on 1 May 1785.
NGC 4619 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
One supernova has been observed in NGC 4619: