NGC 1293 explained
NGC 1293 |
Upright: | 1.15 |
Epoch: | J2000 |
Type: | E0[1] |
Dist Ly: | 65.8Mpc |
H Radial V: | 4173 km/s |
Z: | 0.013920 |
Appmag V: | 14.50 |
Size V: | 1.0 x 1.0 |
Constellation Name: | Perseus |
Names: | CGCG 540-116, MCG +07-07-075, PGC 012597 |
Size: | ~37.8kpc (estimated) |
NGC 1293 is an elliptical galaxy[2] located about 215 million light-years away[3] in the constellation Perseus.[4] It was discovered by astronomer William Herschel on October 17, 1786.[5] NGC 1293 is a member of the Perseus Cluster.[6]
See also
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 1293 . 2018-07-07.
- Web site: Your NED Search Results. ned.ipac.caltech.edu. 2018-07-07.
- Web site: NED Query Results for NGC 1293. ned.ipac.caltech.edu. en-US. 2018-07-07.
- Web site: Revised NGC Data for NGC 1293. spider.seds.org. 2018-07-07.
- 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.