Coma I
Coma I Group | |
---|---|
![]() NGC 4414, a flocculent spiral galaxy in the Coma I Group | |
Observation data (Epoch J2000) | |
Constellation(s) | Coma Berenices & Ursa Major |
Right ascension | 12h 22m 19.4s[1][2] |
Declination | 29° 53′ 47″[1][2] |
Brightest member | NGC 4725[3] |
Number of galaxies | 22–34[3][4][2][5][6] |
Velocity dispersion | 307 km/s[7] |
Redshift | 0.002418 (724 km/s)[1] |
Distance (co-moving) | 14.52 Mpc (47.4 Mly)[7] |
Binding mass | 2.5×1012 [3] M☉ |
X-ray luminosity | 1.6×1043 erg/s [8] |
Other designations | |
Coma I Group,[9] NGC 4274 Group,[1] LGG 279, LGG 294,[4] NBGG 14-01,[1][5] NBGG 14-02, NBGG 14 -2 +1,[9][5] NOGG H 611, NOGG P1 631, NOGG P2 642, NOGG P2 641[2] | |
The Coma I Group is a group of galaxies[3][1] located about 14.5 Mpc (47.3 Mly)[7] away in the constellation Coma Berenices. The brightest member of the group is NGC 4725. The Coma I Group is rich in spiral galaxies while containing few elliptical and lenticular galaxies. Coma I lies in the foreground of the more distant Coma and Leo clusters and is located within the Virgo Supercluster.[3]
The Coma I Group is currently infalling into the Virgo Cluster and will eventually merge with it.[10]
Structure[]
The Coma I Group appears to consist of two main subgroups, a denser subgroup centered on NGC 4274[11] and NGC 4278, and looser one surrounding NGC 4565 as suggested by De Vaucouleurs.[12] However, Gregory and Thompson (1977) found no clear evidence for two distinct subgroups in Coma I. They noted a slight density enhancement around NGC 4274 with the rest of the members of Coma I uniformly distributed to the southeast of this density enhancement. They also noted a central barlike structure with a minor axis of 0.9 Mpc (2.9 Mly) and a major axis of 2.3 Mpc (7.5 Mly).[3] P. Fouque et al. and A. M. Garcia et al. both list the Coma I group consisting of two subgroups centered on NGC 4274 and NGC 4565.[6][4] Additionally, Gibson et al. suggests that another association, the Coma II Group centered on NGC 4725 is associated with the Coma I Group.[9]
Members[]
The table below lists galaxies that have been commonly and consistently identified as group members in the Nearby Galaxies Catalog,[5] the survey of Fouque et al.,[6] the Lyons Groups of Galaxies (LGG) Catalog,[4] and the three group lists created from the Nearby Optical Galaxy sample of Giuricin et al.[2]
Name | Type[13] | R.A. (J2000)[13] | Dec. (J2000)[13] | Redshift (km/s)[13] | Apparent Magnitude[13] |
---|---|---|---|---|---|
SBd? | 11h 58m 56.7s | +30° 24′ 43″ | 760 | 13.1 | |
SA(s)c | 12h 04m 03.8s | +31° 53′ 45″ | 758 | 12.5 | |
SAB(r)c | 12h 09m 17.7s | +29° 55′ 39″ | 609 | 11.69 | |
SBd | 12h 12m 21.4s | +29° 12′ 25″ | 1127 | 13.59 | |
NGC 4203 | SAB0^-? | 12h 15m 05.0s | +33° 11′ 50″ | 1086 | 11.8 |
NGC 4245 | SB0/a?(r) | 12h 17m 36.8s | +29° 36′ 29″ | 884 | 12.31 |
SB0? | 12h 18m 08.2s | +28° 10′ 31″ | 1066 | 11.58 | |
NGC 4274 | (R)SB(r)ab | 12h 19m 50.6s | +29° 36′ 52″ | 930 | 11.34 |
NGC 4278 | E1-2 | 12h 20m 06.8s | +29° 16′ 51″ | 620 | 11.20 |
E0 | 12h 20m 20.8s | +29° 18′ 39″ | 1056 | 13.10 | |
() | (R')SAB0^+(r)? | 12h 22m 26.3s | +29° 12′ 33″ | 913 | 13.22 |
NGC 4314 | SB(rs)a | 12h 22m 31.8s | +29° 53′ 45″ | 963 | 11.43 |
SB(rs)c? | 12h 24m 11.2s | +31° 31′ 19″ | 1253 | 13.6 | |
SABd | 12h 25m 51.2s | +27° 33′ 42″ | 755 | 12.7 | |
NGC 4414 | SA(rs)c? | 12h 26m 27.1s | +31° 13′ 25″ | 716 | 10.96 |
NGC 4448 | SB(r)ab | 12h 28m 15.4s | +28° 37′ 13″ | 661 | 12.00 |
NGC 4494 | E1-2 | 12h 31m 24.1s | +25° 46′ 31″ | 1342 | 10.71 |
Scd? | 12h 33m 51.1s | +30° 16′ 39″ | 1172 | 13.4 | |
NGC 4559 | SAB(rs)cd | 12h 35m 57.6s | +27° 57′ 36″ | 807 | 10.46 |
SB(s)dm? | 12h 35m 34.8s | +25° 51′ 00″ | 1353 | 13.9 | |
NGC 4565 | SA(s)b? | 12h 36m 20.8s | +25° 59′ 16″ | 1230 | 10.42 |
NGC 4725 | SAB(r)ab pec | 12h 50m 26.6s | +25° 30′ 03″ | 1206 | 10.11 |
SBcd? pec | 12h 51m 45.9s | +25° 46′ 37″ | 1190 | 12.96 |
Other possible member galaxies (galaxies listed in only one or two of the lists from the above references) include , , , , NGC 4150, NGC 4308, NGC 4455, , NGC 4534, NGC 4627, NGC 4631, NGC 4656, , , , , , , , and .
Nearby groups[]
The center of the Virgo Cluster (M87) lies about 3.6 Mpc (11.7 Mly) from the Coma I Group.[3]
See also[]
- List of Galaxy Groups
- M94 Group
- M96 Group
- Ursa Major Cluster – Another nearby spiral-rich group within the Virgo Supercluster
References[]
- ^ a b c d e f "Coma I Group". Retrieved 2018-05-12.
- ^ a b c d e G. Giuricin; C. Marinoni; L. Ceriani; A. Pisani (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". Astrophysical Journal. 543 (1): 178–194. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. S2CID 9618325.
- ^ a b c d e f g Gregory, Stephen A.; Thompson, Laird A. (April 1977). "The Coma i Galaxy Cloud". The Astrophysical Journal. 213: 345–350. Bibcode:1977ApJ...213..345G. doi:10.1086/155160. ISSN 0004-637X.
- ^ a b c d A. Garcia (1993). "General study of group membership. II – Determination of nearby groups". Astronomy and Astrophysics Supplement. 100: 47–90. Bibcode:1993A&AS..100...47G.
- ^ a b c d R. B. Tully (1988). Nearby Galaxies Catalog. Cambridge: Cambridge University Press. ISBN 0-521-35299-1.
- ^ a b c P. Fouque; E. Gourgoulhon; P. Chamaraux; G. Paturel (1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members". Astronomy and Astrophysics Supplement. 93: 211–233. Bibcode:1992A&AS...93..211F.
- ^ a b c Boselli, A.; Gavazzi, G. (2009-10-21). "The HI properties of galaxies in the Coma I cloud revisited". Astronomy & Astrophysics. 508 (1): 201–207. arXiv:0909.4140. Bibcode:2009A&A...508..201B. doi:10.1051/0004-6361/200912658. ISSN 0004-6361. S2CID 14049523.
- ^ Garcia-Barreto, J. A.; Downes, D.; Huchtmeier, W. K. (August 1994). "H I deficiency in the Coma I cloud of galaxies" (PDF). Astronomy and Astrophysics. 288: 705–712. Bibcode:1994A&A...288..705G.
- ^ a b c Gibson, Brad K.; Hughes, Shaun M. G.; Stetson, Peter B.; Freedman, Wendy L.; Robert C. Kennicutt, Jr.; Mould, Jeremy R.; Bresolin, Fabio; Ferrarese, Laura; Ford, Holland C. (1999). "The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XVII. The Cepheid Distance to NGC 4725". The Astrophysical Journal. 512 (1): 48. arXiv:astro-ph/9810003. Bibcode:1999ApJ...512...48G. doi:10.1086/306762. ISSN 0004-637X. S2CID 117635398.
- ^ Tully, R. B.; Shaya, E. J. (June 1984). "Infall of galaxies into the Virgo cluster and some cosmological constraints". The Astrophysical Journal. 281: 31–55. Bibcode:1984ApJ...281...31T. doi:10.1086/162073. ISSN 0004-637X.
- ^ "Nearby Groups of Galaxies". ned.ipac.caltech.edu. Retrieved 2018-05-19.
- ^ Forbes, Duncan A. (October 1996). "Globular Cluster Luminosity Functions and the Hubble Constant From WFPC Imaging: Galaxies in the Coma I Cloud". The Astronomical Journal. 112: 1409. arXiv:astro-ph/9611139. Bibcode:1996AJ....112.1409F. doi:10.1086/118108. ISSN 0004-6256. S2CID 118922735.
- ^ a b c d e "NASA/IPAC Extragalactic Database". Results for various galaxies. Retrieved 2006-10-15.
- Virgo Supercluster
- Coma Berenices
- Galaxy clusters
- Ursa Major (constellation)
- Coma I Group