NGC 1334 explained

NGC 1334
Upright:1.15
Epoch:J2000
Type:Sbc pec[1]
Dist Ly:56.4Mpc
H Radial V:4274 km/s
Z:0.014257
Appmag V:14.1
Size V:1.5 x 0.7
Constellation Name:Perseus
Names:UGC 02759, CGCG 541-017, MCG +07-08-018, PGC 013001
Size:~25kpc (estimated)

NGC 1334 is a spiral galaxy[2] located about 185 million light-years away in the constellation Perseus.[3] It was discovered by astronomer Heinrich d'Arrest on February 14, 1863.[4] NGC 1334 is a member of the Perseus Cluster[5] [6] and is a starburst galaxy. It also appears to have a complex distorted structure.[7]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 1334 . 2018-07-08.
  2. Web site: HyperLeda -object description. leda.univ-lyon1.fr. 2018-07-08.
  3. Web site: Revised NGC Data for NGC 1334. spider.seds.org. 2018-07-08.
  4. Web site: New General Catalog Objects: NGC 1300 - 1349. cseligman.com. en-US. 2018-07-08.
  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: Hierarchy catalogue. leda.univ-lyon1.fr. 2018-07-08.
  7. H.. Meusinger. J.. Brunzendorf. R.. Krieg. November 2000. IRAS galaxies in the Perseus cluster. Astronomy and Astrophysics. en. 363. 933. 0004-6361. 2000A&A...363..933M.