NGC 4179 explained
Epoch: | J2000 |
Constellation Name: | Virgo |
H Radial V: | 1230 km/s |
Z: | 0.00411 |
Dist Ly: | [1] |
Group Cluster: | Virgo Cluster |
Type: | S0[2] |
Appmag B: | 12.8 |
Names: | [3] |
NGC 4179 is a lenticular galaxy located in the constellation Virgo. It was discovered by William Herschel on January 14, 1784.[4] It is a member of the NGC 4179 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.[3] [5]
Notes and References
- 10.1111/j.1365-2966.2007.11790.x. astro-ph/0703768. 2007MNRAS.378..594P. On the three-dimensional structure of edge-on disc galaxies. 2007. Pohlen. Michael. Zaroubi. Saleem. Peletier. Reynier F.. Dettmar. Ralf-Jürgen. Monthly Notices of the Royal Astronomical Society. 378. 2. 594–616. free . 14858064.
- 10.1093/mnras/stt296. 1302.3853. 2013MNRAS.431.1823M. A spectral atlas of H II galaxies in the near-infrared. 2013. Martins. Lucimara P.. Rodríguez-Ardila. Alberto. Diniz. Suzi. Gruenwald. Ruth. De Souza. Ronaldo. Monthly Notices of the Royal Astronomical Society. 431. 2. 1823–1839. free .
- NGC 4179. 2021-04-12.
- Web site: New General Catalog Objects: NGC 4150 - 4199. cseligman.com.
- Web site: The Virgo III Groups . Atlas of the Universe . 2010-11-27 .