NGC 254 explained

NGC 254
Epoch:J2000
Constellation Name:Sculptor
Ra:[1]
Z:0.005434[2]
H Radial V:1629
Dist Ly:17.1Mpc
Type:(R)SA(rl)0+
Appmag V:11.82
Appmag B:11.62
Size V:2.6 × 1.7[3]
Names:MCG-05-03-005, PGC 2778

NGC 254 is a lenticular galaxy located in the constellation Sculptor. It was discovered by John Herschel in 1834.[3] It is in a galaxy group with NGC 134.

NGC 254 is an example of a ring galaxy, a galaxy with a ring, and in this case, no central bar. Across the entire galaxy disk, there is a disk of ionized gas rotating in the direction opposite the stellar disk's rotation. This situation may have arose when a retrograde-orbiting satellite galaxy accreted onto the galaxy itself, some 1 billion years ago.[4]

See also

Notes and References

  1. NGC 254. 12 February 2017.
  2. Web site: NASA/IPAC Extragalactic Database. Results for NGC 254. 2 September 2016.
  3. Web site: New General Catalog Objects: NGC 250 - 299. cseligman.com. 12 February 2017.
  4. 10.1051/0004-6361/202141934. Star formation in outer rings of S0 galaxies. IV. NGC 254: A double-ringed S0 with gas counter-rotation. 2022. Katkov. Ivan Yu.. Kniazev. Alexei Yu.. Sil'Chenko. Olga K.. Gasymov. Damir. Astronomy & Astrophysics. 658. A154. 2112.03289. 245728982. 2022A&A...658A.154K.