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  • 21 Aug, 2019

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NGC 1585

NGC 1585 is a spiral galaxy in the constellation of Caelum. Its velocity with respect to the cosmic microwave background is 4,635 ± 31 km/s, which corresponds to a Hubble distance of 68.4 ± 4.8 Mpc (∼223 million light-years). It was discovered by British astronomer John Herschel on 1 December 1837.

The SIMBAD database lists NGC 1585 as a Seyfert I Galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.

One supernova has been observed in NGC 1585: SN 2023vio (type Iax [02cx-like], mag. 19.053) was discovered by ATLAS on 17 October 2023.

See also

References

  1. ^ "NASA/IPAC Extragalactic Database". Results for NGC 1585. Retrieved 19 July 2024.
  2. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 1585". Celestial Atlas. Retrieved 12 December 2024.
  3. ^ "NGC 1585". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 12 December 2024.
  4. ^ "SN 2023vio". Transient Name Server. IAU. Retrieved 12 December 2024.