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NGC 4598
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| NGC 4598 | |
|---|---|
 Sloan Digital Sky Survey image of NGC 4598. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 40m 11.9s[1] |
| Declination | 08° 23′ 01″[1] |
| Redshift | 0.006541[1] |
| Heliocentric radial velocity | 1961 km/s[1] |
| Distance | 63.7 Mly (19.54 Mpc),[2] 88.71 Mly (27.200 Mpc), 102 Mly (31.3 Mpc) (Redshift-based) [1][2] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 13.6[1] |
| Characteristics | |
| Type | SB0[1] |
| Size | ~43,900 ly (13.45 kpc) (estimated)[1] |
| Apparent size (V) | 1.47 x 1.06[1] |
| Other designations | |
| CGCG 70-207, MCG 2-32-171, PGC 42427, UGC 7829, VCC 1827[1] | |
NGC 4598 is a barred lenticular galaxy[3] located in the constellation Virgo.[4] NGC 4598 was discovered by astronomer William Herschel on April 15, 1784.[5] The distance to NGC 4598 has not been accurately determined; measurements vary from 64 to 102 million light-years.[3][6] According to the NASA/IPAC Extragalactic Database, its redshift based distance is 102 Mly (31.3 Mpc) while its redshift independent based distance is 88.71 Mly (27.200 Mpc).[3] Also, according to SIMBAD, its distance is 63.7 Mly (19.54 Mpc).[6] NGC 4598's average distance is 84.8 Mly (26.0 Mpc).[1] NGC 4598 is usually considered to be a member of the Virgo Cluster.[7][8] However, P. Fouqu´e et al. suggests it may be a background galaxy independent of the main cluster.[9]
See also
[edit]Notes
[edit]- 1.^ This value was determined by using the three other measured values given above.
References
[edit]- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4598. Retrieved 2018-03-18.
- ^ a b "NGC 4598". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-03-18.
- ^ a b c "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-03-19.
- ^ "Revised NGC Data for NGC 4598". spider.seds.org. Retrieved 2018-03-19.
- ^ "New General Catalog Objects: NGC 4550 - 4599". cseligman.com. Retrieved 2018-03-08.
- ^ a b "NGC 4598". Retrieved 2018-03-19.
- ^ Binggeli, B.; Sandage, A.; Tammann, G. A. (1985-09-01). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area". The Astronomical Journal. 90: 1681–1759. Bibcode:1985AJ.....90.1681B. doi:10.1086/113874. ISSN 0004-6256.
- ^ Erwin, Peter; Gutiérrez, Leonel; Beckman, John E. (2012). "A Strong Dichotomy in S0 Disk Profiles between the Virgo Cluster and the Field". The Astrophysical Journal Letters. 744 (1): L11. arXiv:1111.5027. Bibcode:2012ApJ...744L..11E. doi:10.1088/2041-8205/744/1/l11. ISSN 2041-8205. S2CID 119187927.
- ^ Fouqué, P.; Solanes, J. M.; Sanchis, T.; Balkowski, C. (2001-09-01). "Structure, mass and distance of the Virgo cluster from a Tolman-Bondi model". Astronomy & Astrophysics. 375 (3): 770–780. arXiv:astro-ph/0106261. Bibcode:2001A&A...375..770F. doi:10.1051/0004-6361:20010833. ISSN 0004-6361. S2CID 10468717.
External links
[edit]
Wikimedia Commons has media related to NGC 4598.
- NGC 4598 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
