NGC 1892

Spiral galaxy in the constellation Dorado
NGC 1892
NGC 1892 imaged by the Hubble Space Telescope
Observation data (2000.0 epoch)
ConstellationDorado
Right ascension05h 17m 9.0s[1]
Declination−64° 57′ 35″[1]
Redshift0.004546[1]
Heliocentric radial velocity1363 km/s[1]
Distance50,000,000 ly (15,500,000 pc)[2]
Apparent magnitude (V)12.2[3]
Characteristics
TypeScd[2]
Apparent size (V)2.9' × 0.8'[3]
Other designations
MCG+03-01-030, 2MFGC 4320, 2MASX J05170905-6457354, IRAS 05169-6500, PGC 17042[4]

NGC 1892 is a spiral galaxy in the constellation Dorado. It was discovered November 30, 1834 by John Herschel.

A probable supernova of type IIP was photographed by the Carnegie-Irvine Galaxy Survey (CGS) in 2004,[5] but it was not noticed until Brazilian amateur astronomer Jorge Stockler de Moraes compared the CGS image to one he took in January 2017.[6]

References

  1. ^ a b c d "NED results for object NGC 1892". NASA/IPAC EXTRAGALACTIC DATABASE. Caltech. Retrieved 29 September 2018.
  2. ^ a b Guillochon, James; Stockler de Moraes, Jorge; Nicholl, Matt; Patnaude, Daniel J; Auchetti, Katie; Barth, Aaron J; Ho, Luis C; Li, Zhao-Yu; Carnegie-Irvine Galaxy Survey (2018). "Serendipitous Discovery of a 14 year old Supernova at 16 Mpc". Research Notes of the AAS. 2 (3): 165. arXiv:1809.00163. Bibcode:2018RNAAS...2..165G. doi:10.3847/2515-5172/aade89. S2CID 119431988.
  3. ^ a b Seligman, Courtney. "Celestial Atlas NGC Objects 1850-1899". cseligman.com. Retrieved 29 September 2018.
  4. ^ "NGC 1892". SIMBAD. Retrieved 29 September 2018.
  5. ^ "NGC 1892". The Carnegie-Irvine Galaxy Survey (CGS). Retrieved 29 September 2018.
  6. ^ Kohler, Susanna (2018). "Surprise Discovery of a 14-Year-Old Supernova". Aas Nova Highlights: 4028. Bibcode:2018nova.pres.4028K. Retrieved 29 September 2018.

External links

  • Media related to NGC 1892 at Wikimedia Commons
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