NGC 1282 explained
NGC 1282 |
Upright: | 1.15 |
Epoch: | J2000 |
Type: | E[1] |
Dist Ly: | 70Mpc |
H Radial V: | 2,139 km/s |
Z: | 0.007135 |
Appmag V: | 13.87 |
Size V: | 1.4 x 1.1 |
Constellation Name: | Perseus |
Names: | CGCG 540-109, MCG 7-7-68, PGC 12471, UGC 2675 |
Size: | ~35.3kpc (estimated) |
NGC 1282 is an elliptical galaxy[2] located about 230 million light-years away[3] in the constellation Perseus.[4] It was discovered by astronomer Guillaume Bigourdan on October 23, 1884.[5] NGC 1282 is a member of the Perseus Cluster.[5] [6]
A type Ia supernova designated as SN 2008fh was detected near NGC 1282[7] on either July 30,[7] [8] or August 30, 2008.[9] [10] Oddly, though, the supernova was not associated with the galaxy.[8]
See also
Notes and References
- Web site: NASA/IPAC Extragalactic Database. Results for NGC 1282. 2018-07-06.
- Web site: Your NED Search Results. ned.ipac.caltech.edu. 2018-07-07.
- Web site: NED Query Results for NGC 1282. ned.ipac.caltech.edu. en-US. 2018-07-07.
- Web site: Revised NGC Data for NGC 1282. 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.
- Web site: Bright Supernovae - 2008.. rochesterastronomy.org. 2018-07-07.
- Web site: ATel #1690: Discovery of a probably sub-luminous type Ia supernova ROTSE3 J032048.6+412145. ATel. 2018-07-07.
- Web site: SN 2008fh Transient Name Server. wis-tns.weizmann.ac.il. en. 2018-07-07.
- Web site: 2008fh - The Open Supernova Catalog. sne.space. en-US. 2018-07-07. 2018-07-07. https://web.archive.org/web/20180707090448/https://sne.space/sne/2008fh/. dead.