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.
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