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

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 1267 . 2018-06-18.
  2. Web site: Your NED Search Results. ned.ipac.caltech.edu. 2018-06-18.
  3. Web site: Revised NGC Data for NGC 1267. spider.seds.org. 2018-06-18.
  4. Web site: New General Catalog Objects: NGC 1250 - 1299. cseligman.com. en-US. 2018-06-15.
  5. 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.
  6. Web site: New General Catalog Objects: NGC 1250 - 1299. cseligman.com. en-US. 2018-06-18.