NGC 214
HST image of NGC 214
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension00h 41m 28.02246s[1]
Declination+25° 29′ 57.8430″[1]
Redshift0.015134[2]
Heliocentric radial velocity4,555 km/s[3]
Distance193.8 Mly (59.43 Mpc)[3]
Apparent magnitude (V)12.97[2]
Characteristics
TypeSABbc[4]
Apparent size (V)1.9' × 1.4'[2]
Other designations
UGC 438, MCG +04-02-044, IRAS 00387+2513, F00388+2513,[5] CGCG 479-059, 2MASX J00412801+2529576, 2MASXi J0041280+252957, PGC 2479.[2]

NGC 214 is a spiral galaxy in the northern constellation of Andromeda, located at a distance of 194 megalight-years from the Milky Way.[3] It was discovered on September 10, 1784 by William Herschel.[6] The shape of this galaxy is given by its morphological classification of SABbc,[4] which indicates a weak bar-like structure (SAB) at the core and moderate to loosely-wound spiral arms (bc).

On July 19, 2005, a magnitude 17.4 supernova was detected at a position 16″ west and 2″ north of the galactic nucleus. The object was not visible on plates taken July 2, so it likely erupted after that date.[7] Designated SN 2005db, it was determined to be a type IIn supernova based on the spectrum.[8] A second supernova event was spotted from an image taken August 30, 2006, at 43″ west and 11.3″ south of the nucleus. It reached magnitude 17.8 and was designated SN 2006ep.[9] This was determined to be a type-Ib/c supernova.[10]

References

  1. 1 2 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. 1 2 3 4 "NASA/IPAC Extragalactic Database". Results for NGC 0214. Retrieved 2016-09-02.
  3. 1 2 3 Tully, R. Brent; et al. (2016). "Cosmicflows-3". The Astronomical Journal. 152 (2): 50. arXiv:1605.01765. Bibcode:2016AJ....152...50T. doi:10.3847/0004-6256/152/2/50. S2CID 250737862.
  4. 1 2 García-Lorenzo, B.; et al. (January 2015). "Ionized gas kinematics of galaxies in the CALIFA survey. I. Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems". Astronomy & Astrophysics. 573: 43. arXiv:1408.5765. Bibcode:2015A&A...573A..59G. doi:10.1051/0004-6361/201423485. S2CID 55475658. A59.
  5. ↑ "NGC 214". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved March 27, 2020.
  6. ↑ "New General Catalog Objects: NGC 200 - 249". Cseligman. Retrieved September 15, 2016.
  7. ↑ Monard, L. A. G. (July 2005). Green, D. W. E. (ed.). "Supernova 2005db in NGC 214". Central Bureau Electronic Telegrams. 182: 1. Bibcode:2005CBET..182....1M.
  8. ↑ Blanc, N.; et al. (July 2005). Green, D. W. E. (ed.). "Supernova 2005db in NGC 214". Central Bureau Electronic Telegrams. 183: 1. Bibcode:2005CBET..183....1B.
  9. ↑ Joubert, N.; et al. (August 2006). Green, D. W. E. (ed.). "Supernova 2006ep in NGC 214". Central Bureau Electronic Telegrams. 609: 1. Bibcode:2006CBET..609....1J.
  10. ↑ Joubert, N.; et al. (September 2006). Green, D. W. E. (ed.). "Supernovae 2006ep, 2006eq, 2006er". IAU Circular. 8744: 2. Bibcode:2006IAUC.8744....2J.
  • Media related to NGC 214 at Wikimedia Commons
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.