NGC 1264 explained
NGC 1264 |
Upright: | 1.15 |
Epoch: | J2000 |
Type: | SBab[1] |
Dist Ly: | 44.7Mpc |
H Radial V: | 3246 km/s |
Z: | 0.010827 |
Appmag V: | 16.0 |
Size V: | 1.2 x 1.1 |
Constellation Name: | Perseus |
Names: | MCG 7-7-50, PGC 12270, UGC 2643 |
Size: | ~15.41kpc (estimated) |
NGC 1264 is a low-surface-brightness[2] barred spiral galaxy[3] located about 145 million light-years away in the constellation Perseus.[4] The galaxy was discovered by astronomer Guillaume Bigourdan on October 19, 1884.[5] NGC 1264 is a member of the Perseus Cluster.[6]
See also
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 1264 . 2018-06-16.
- News: NGC 1264. 2018-06-17.
- Web site: Your NED Search Results. ned.ipac.caltech.edu. 2018-06-17.
- Web site: Revised NGC Data for NGC 1264. spider.seds.org. 2018-06-17.
- Web site: New General Catalog Objects: NGC 1250 - 1299. cseligman.com. en-US. 2018-06-15.
- Brunzendorf. J.. Meusinger. H.. October 1, 1999. The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types. Astronomy and Astrophysics Supplement Series. en. 139. 1. 141–161. 10.1051/aas:1999111. 0365-0138. 1999A&AS..139..141B. free.