NGC 4038 Group | |
---|---|
Observation data (Epoch J2000) | |
Constellation(s) | Corvus and Crater |
Right ascension | [1][2] |
Declination | [1][2] |
Number of galaxies | 13-27[3][4][1][2] |
Brightest member | Antennae Galaxies |
Other designations | |
LGG 263,[1] NOGG H 580,[2] NOGG P1 596,[2], NOGG P2 603[2] |
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See also: Galaxy groups and clusters, List of galaxy clusters | |
The NGC 4038 Group is a group of galaxies in the constellations Corvus and Crater. The group may contain between 13 and 27 galaxies. The group's best known galaxies are the Antennae Galaxies (NGC 4038/NGC4039), a well-known interacting pair of galaxies.
The table below lists galaxies that have been consistently identified as group members in the Nearby Galaxies Catalog,[3] the survey of Fouque et al.,[4] the Lyons Groups of Galaxies (LGG) Catalog,[1] and the three group lists created from the Nearby Optical Galaxy sample of Giuricin et al.[2]
Name | Type[5] | R.A. (J2000)[5] | Dec. (J2000)[5] | Redshift (km/s)[5] | Apparent Magnitude[5] |
---|---|---|---|---|---|
Antennae Galaxies (NGC 4038/NGC 4039) | 12h 01m 53.3s | -18° 52′ 30″ | 1705 ± 5 | 13.0 | |
NGC 3956 | SA(s)c | 11h 54m 00.7s | -20° 34′ 02″ | 1645 ± 5 | 13.1 |
NGC 3957 | SA0 | 11h 54m 01.5s | -19° 34′ 08″ | 1637 ± 19 | 13.1 |
NGC 3981 | SAB(s)bc pec | 11h 56m 07.5s | -19° 53′ 46″ | 1723 ± 4 | 12.1 |
NGC 4024 | SB0 | 11h 58m 31.2s | -18° 20′ 49″ | 1694 ± 15 | 13.2 |
NGC 4027 | SB(s)dm | 11h 59m 30.2s | -19° 15′ 55″ | 1671 ± 6 | 11.7 |
NGC 4033 | E6 | 12h 00m 34.7s | -17° 50′ 33″ | 1617 ± 20 | 13.2 |
NGC 4050 | SB(r)ab | 12h 02m 54.0s | -16° 22′ 25″ | 1761 ± 8 | 13.1 |
PGC 37476 | SB(rs)c | 11h 55m 50.6s | -18° 11′ 47″ | 1596 ± 8 | 14.0 |
PGC 38087 | SB(s)cd | 12h 03m 24.4s | -19° 31′ 21″ | 1664 ± 7 | 15.0 |
UGCA 254 | SAB(s)cd | 11h 54m 49.5s | -16° 51′ 50″ | 1813 ± 6 | 14.5 |
UGCA 257 | SB(s)m | 11h 58m 25.4s | -22° 26′ 24″ | 1795 ± 5 | 13.6 |
Additionally, the references above frequently but inconsistently identify PGC 37513, PGC 37565, and UGCA 270 as members of this group. Based on the above references, the exact membership of this group is somewhat uncertain as is the exact number of galaxies within the group.