NGC 830 explained
NGC 830 |
Epoch: | J2000 |
Constellation Name: | Cetus |
Z: | 0.01349 |
H Radial V: | 4017 km/s |
Dist Ly: | [1] |
Type: | SB0-?[2] |
Appmag B: | 15.0 |
Names: | [3] |
NGC 830 is a barred lenticular galaxy in the constellation Cetus. It is estimated to be about 170 million light-years from the Milky Way[1] and has a diameter of approximately 70,000 light years.[4] [5] [6]
See also
References
- Groups of Galaxies in the Two Micron All Sky Redshift Survey. Crook, Aidan C.. Huchra, John P.. Martimbeau, Nathalie. Masters, Karen L.. Jarrett, Tom. Macri, Lucas M.. The Astrophysical Journal. 655. 2. 790–813. 2007. 2007ApJ...655..790C. 10.1086/510201. astro-ph/0610732. 11672751 .
- Web site: Results for object NGC 0830 (NGC 830). NASA/IPAC Extragalactic Database. California Institute of Technology. 2020-05-24.
- NGC 830. 2020-05-24.
- Web site: The galaxy NGC 830 - In-The-Sky.org. Ford. Dominic. in-the-sky.org. en. 2020-03-18.
- Web site: Your NED Search Results. ned.ipac.caltech.edu. 2020-03-18.
- Web site: Revised NGC Data for NGC 830. spider.seds.org. 2020-03-18.