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NGC 1268 is a spiral galaxy located about 140 million light-years away[2] in the constellation Perseus.[3] It was discovered by astronomer Heinrich d'Arrest on February 14, 1863.[4] NGC 1268 is a member of the Perseus Cluster[5][4] and appears to show signs of distortion in the form of bridges.[5] These features may be the result of a strong interaction with NGC 1267.[5][4]
On August 30, 2008, a type Ia supernova designated as SN 2008fg was discovered in NGC 1268.[6][7][8]
^ abcdefghij"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.
^ abc"New General Catalog Objects: NGC 1250 - 1299". cseligman.com. Retrieved 2018-06-15.
^ abcBrunzendorf, 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.
NGC1268 is a spiral galaxy located about 140 million light-years away in the constellation Perseus. It was discovered by astronomer Heinrich d'Arrest...
1863. NGC 1267 is a member of the Perseus Cluster and is possibly interacting with the spiral galaxy NGC1268. List of NGC objects (1001–2000) NGC 4567...
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