NGC 1267 explained
NGC 1267 |
Upright: | 1.15 |
Epoch: | J2000 |
Type: | cD, E+[1] |
Dist Ly: | 67Mpc |
H Radial V: | 5059 km/s |
Z: | 0.016875 |
Appmag V: | 15.4 |
Size V: | 1.1 x 0.9 |
Constellation Name: | Perseus |
Names: | CGCG 540-92, MCG 7-7-55, PGC 12331, UGC 2657 |
Size: | ~26.14kpc (estimated) |
NGC 1267 is an elliptical galaxy located about 220 million light-years away[2] in the constellation Perseus.[3] NGC 1267 was discovered by astronomer Heinrich d'Arrest on February 14, 1863.[4] NGC 1267 is a member of the Perseus Cluster[5] and is possibly interacting with the spiral galaxy NGC 1268.[6]
See also
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 1267 . 2018-06-18.
- Web site: Your NED Search Results. ned.ipac.caltech.edu. 2018-06-18.
- Web site: Revised NGC Data for NGC 1267. spider.seds.org. 2018-06-18.
- 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.
- Web site: New General Catalog Objects: NGC 1250 - 1299. cseligman.com. en-US. 2018-06-18.