NGC 1250 explained

NGC 1250
Upright:	1.15
Epoch:	J2000
Type:	S0^0^[1]
Dist Ly:	84.5Mpc
H Radial V:	6014 km/s
Z:	0.020061
Appmag V:	13.96
Size V:	2.1 x 0.9
Constellation Name:	Perseus
Names:	UGC 2613, MCG +07-07-040, PGC 12098

NGC 1250 is an edge-on lenticular galaxy located about 275 million light-years away^[2] in the constellation Perseus.^[3] It was discovered by astronomer Lewis Swift on Oct 21, 1886.^[4] NGC 1250 is a member of the Perseus Cluster.^[5]

See also

• List of NGC objects (1001–2000)
• NGC 1277

Notes and References

1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 1250 . 2018-06-15.
2. Web site: Your NED Search Results. ned.ipac.caltech.edu. 2018-06-15.
3. Web site: Revised NGC Data for NGC 1250. spider.seds.org. 2018-06-15.
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.