NGC 4478 is an elliptical galaxy located about 50 million light-years away[3] in the constellation Virgo.[4] NGC 4478 was discovered by astronomer William Herschel on April 12, 1784.[5] NGC 4478 is a member of the Virgo Cluster.[6]
| NGC 4478 | |
|---|---|
 SDSS image of NGC 4478. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 30m 17.4s[1] |
| Declination | 12° 19′ 43″[1] |
| Redshift | 0.004500/1349 km/s[1] |
| Distance | 52.2 Mly[2] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 12.36[1] |
| Characteristics | |
| Type | E2[1] |
| Size | ~30,000 ly (estimated)[1] |
| Apparent size (V) | 1.9 x 1.6[1] |
| Other designations | |
| CGCG 70-133, MCG 2-32-99, PGC 41297, UGC 7645, VCC 1279[1] | |
Nuclear disk
editHubble images indicate that NGC 4478 has a central nuclear disk.[7]
Metallicity
editIn NGC 4478, the central regions of the galaxy are high in metals while having less overabundance of the element iron than the main body. In contrast, the outer regions of the galaxy are low in metals while having a high overabundance in iron.[7]
Globular clusters
editNGC 4478 has a typical sub-population of metal-poor globular clusters. However, it has a lack of metal-rich clusters. The lack of metal-rich clusters in other galaxies is usually attributed to accretion, or mergers with other galaxies. The only other known elliptical that has been shown to have a domination of metal-poor globular clusters is the giant galaxy NGC 4874 which is located in the center of the Coma Cluster.[2]
Reduced population
editDue to tidal truncation caused by Messier 87, a significant amount of globular clusters have been striped away from NGC 4478 and have become members of Messier 87's globular cluster system.[8]
Interaction with Messier 87
editNGC 4478 is likely to be a companion of the giant elliptical Messier 87. The two galaxies are separated from each other by about 130,400 Light-years (40 kpc). NGC 4478 has been tidally truncated by Messier 87.[2]
See also
editReferences
edit- ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 4478. Retrieved 2017-10-15.
- ^ a b c Kissler-Patig, M.; Brodie, J. P.; Minniti, D. (4 June 2002). "Extragalactic globular clusters in the near infrared. I. A comparison between M87 and NGC 4478" (PDF). Astronomy & Astrophysics. 391 (2): 441–452. arXiv:astro-ph/0206140. Bibcode:2002A&A...391..441K. doi:10.1051/0004-6361:20020831. S2CID 16529462.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-10-15.
- ^ Rojas, Sebastián García. "Galaxy NGC 4478 - Elliptical Galaxy in Virgo Constellation · Deep Sky Objects Browser". DSO Browser. Retrieved 2017-10-15.
- ^ "New General Catalog Objects: NGC 4450 - 4499". cseligman.com. Retrieved 2017-10-08.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2017-10-15.
- ^ a b Morelli, L.; Halliday, C.; Corsini, E. M.; Pizzella, A.; Thomas, D.; Saglia, R. P.; Davies, R. L.; Bender, R.; Birkinshaw, M.; Bertola, F. (19 July 2004). "Nuclear stellar discs in low-luminosity elliptical galaxies: NGC 4458 and 4478" (PDF). Monthly Notices of the Royal Astronomical Society. 354 (3): 753–762. arXiv:astro-ph/0408084. Bibcode:2004MNRAS.354..753M. doi:10.1111/j.1365-2966.2004.08236.x. S2CID 13933949.
- ^ NEILSEN, JR., ERIC H.; TSVETANOV, ZLATAN I.; FORD, HOLLAND C. (6 February 1997). "The Surface Brightness Fluctuations and Globular Cluster Population of NGC 4478". The Astrophysical Journal. 483 (2): 745–753. arXiv:astro-ph/9712339. Bibcode:1997ApJ...483..745N. doi:10.1086/304267. S2CID 15606310.
External links
edit
- NGC 4478 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images