Summary
NGC 4580 is an unbarred spiral galaxy[2] located about 70 million light-years away[3] in the constellation Virgo.[4] NGC 4580 is also classified as a LINER galaxy.[3][5] It was discovered by astronomer William Herschel on February 2, 1786[6] and is a member of the Virgo Cluster.[2][7]
| NGC 4580 | |
|---|---|
 SDSS image of NGC 4580 | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 37m 48.4s[1] |
| Declination | 05° 22′ 07″[1] |
| Redshift | 0.003449[1] |
| Heliocentric radial velocity | 1034 km/s[1] |
| Distance | 69.35 Mly (21.263 Mpc)[1] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 12.7[1] |
| Characteristics | |
| Type | SAB(rs)a pec, LINER[1] |
| Size | ~52,400 ly (16.08 kpc) (estimated)[1] |
| Apparent size (V) | 2.28 x 1.45[1] |
| Other designations | |
| CGCG 42-183, IRAS 12352+0538, MCG 1-32-117, PGC 42174, UGC 7794, VCC 1730[1] | |
Physical characteristics edit
NGC 4580 consists of a ringed structure. The inner pseudoring of the galaxy is very well-defined and is made of two tightly wound spiral arms. Three very diffuse spiral arms which are partly defined by dust, split off from the inner pseudoring.[2]
Truncated disk edit
NGC 4580 has a severely truncated star-forming disk. This may be due to ram-pressure stripping[2] caused by the infall of the Messier 49 subcluster into the Virgo Cluster.[8] Due to the truncation of the star forming disk, NGC 4580 is classified as an anemic galaxy.[9]
See also edit
References edit
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4580. Retrieved 2018-02-24.
- ^ a b c d "NGC 4580 - SA(rs)ab". The de Vaucouleurs Atlas of Galaxies. Retrieved 2018-02-24.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-02-24.
- ^ "Revised NGC Data for NGC 4580". spider.seds.org. Retrieved 2018-02-24.
- ^ "NGC4580". Retrieved 2018-02-24.
- ^ "New General Catalog Objects: NGC 4550 - 4599". cseligman.com. Retrieved 2018-02-24.
- ^ "The Virgo Cluster". www.atlasoftheuniverse.com. Retrieved 2018-02-24.
- ^ Cortés, Juan R.; Kenney, Jeffrey D. P.; Hardy, Eduardo (2008). "Distances from Stellar Kinematics for Peculiar Virgo Cluster Spiral Galaxies". The Astrophysical Journal. 683 (1): 78. arXiv:0803.3638. Bibcode:2008ApJ...683...78C. doi:10.1086/588604. ISSN 0004-637X. S2CID 14426987.
- ^ Koopmann, Rebecca A.; Kenney, Jeffrey D. P. (2004). "Hα Morphologies and Environmental Effects in Virgo Cluster Spiral Galaxies". The Astrophysical Journal. 613 (2): 866–885. arXiv:astro-ph/0406243. Bibcode:2004ApJ...613..866K. doi:10.1086/423191. ISSN 0004-637X. S2CID 17519217.
External links edit
- NGC 4580 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images