NGC 1268
NGC 1268 is a spiral galaxy located about 140 million light-years away in the constellation Perseus. It was discovered by astronomer Heinrich d'Arrest on February 14, 1863. NGC 1268 is a member of the Perseus Cluster and appears to show signs of distortion in the form of bridges. These features may be the result of a strong interaction with NGC 1267.
On August 30, 2008, a type Ia supernova designated as SN 2008fg was discovered in NGC 1268.
See also
References
- ^ "NASA/IPAC Extragalactic Database". Results for NGC 1268. Retrieved 2018-06-19.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-06-19.
- ^ "Revised NGC Data for NGC 1268". spider.seds.org. Retrieved 2018-06-19.
- ^ "New General Catalog Objects: NGC 1250 - 1299". cseligman.com. Retrieved 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. 139 (1): 141–161. Bibcode:1999A&AS..139..141B. doi:10.1051/aas:1999111. ISSN 0365-0138.
- ^ "List of supernovae sorted by host name". Bright Supernova - Archives. Retrieved 2018-06-19.
- ^ "SN 2008fg | Transient Name Server". wis-tns.weizmann.ac.il. Retrieved 2018-06-19.
- ^ "2008fg - The Open Supernova Catalog". sne.space. Archived from the original on 2018-06-20. Retrieved 2018-06-19.
External links
Media related to NGC 1268 at Wikimedia Commons- NGC 1268 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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