ESO 306-17 | |
---|---|
Observation data ( J2000.0 epoch) | |
Constellation | Columba |
Right ascension | 05h 40m 06.73s [1] |
Declination | −40° 50′ 10.6″ [1] |
Redshift | 0.035805±0.000083 [2] |
Heliocentric radial velocity | 10,734±25 km/s [2] |
Galactocentric velocity | 10,544±26 km/s [2] |
Distance | 517.3 ± 36.20
Mly (158.6 ± 11.1
Mpc)h−1 0.6774 (Comoving) [2] 506 Mly (155.1 Mpc)h−1 0.6774 ( Light-travel) |
Apparent magnitude (B) | 13.36 [1] |
Characteristics | |
Type | E+3 [2] |
Size | 1,070,000
ly × 706,100 ly (328.04 kpc × 216.50 kpc) ( diameter; 90% total B-band light) [2] [a] 399,300 ly × 287,500 ly (122.42 kpc × 88.15 kpc) ( diameter; "total" magnitude) [2] [a] |
Apparent size (V) | 2.5 ′ × 1.5 ′ ( V-band) [2] |
Other designations | |
MCG -07-12-009, PGC 17570 [3] |
ESO 306-17 is a fossil group giant elliptical galaxy in the Columba constellation, about 1.07 million light-years in diameter, [2] [4] and roughly 517 million light-years away. [2]
The galaxy is situated alone in a volume of space about it. It is theorized that the galaxy cannibalized its nearest companions, hence, being a fossil group. [5] The galaxy is a giant elliptical of type cD3 [2] (E+3), one of the largest types of galaxies.
ESO 306-17 | |
---|---|
Observation data ( J2000.0 epoch) | |
Constellation | Columba |
Right ascension | 05h 40m 06.73s [1] |
Declination | −40° 50′ 10.6″ [1] |
Redshift | 0.035805±0.000083 [2] |
Heliocentric radial velocity | 10,734±25 km/s [2] |
Galactocentric velocity | 10,544±26 km/s [2] |
Distance | 517.3 ± 36.20
Mly (158.6 ± 11.1
Mpc)h−1 0.6774 (Comoving) [2] 506 Mly (155.1 Mpc)h−1 0.6774 ( Light-travel) |
Apparent magnitude (B) | 13.36 [1] |
Characteristics | |
Type | E+3 [2] |
Size | 1,070,000
ly × 706,100 ly (328.04 kpc × 216.50 kpc) ( diameter; 90% total B-band light) [2] [a] 399,300 ly × 287,500 ly (122.42 kpc × 88.15 kpc) ( diameter; "total" magnitude) [2] [a] |
Apparent size (V) | 2.5 ′ × 1.5 ′ ( V-band) [2] |
Other designations | |
MCG -07-12-009, PGC 17570 [3] |
ESO 306-17 is a fossil group giant elliptical galaxy in the Columba constellation, about 1.07 million light-years in diameter, [2] [4] and roughly 517 million light-years away. [2]
The galaxy is situated alone in a volume of space about it. It is theorized that the galaxy cannibalized its nearest companions, hence, being a fossil group. [5] The galaxy is a giant elliptical of type cD3 [2] (E+3), one of the largest types of galaxies.