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.[2]

NGC 1585
The spiral galaxy NGC 1585.
Observation data (J2000 epoch)
ConstellationCaelum
Right ascension04h 27m 33.0055s[1]
Declination−42° 09′ 54.502″[1]
Redshift0.015534[1]
Heliocentric radial velocity4657 ± 31 km/s[1]
Distance223.0 ± 15.8 Mly (68.36 ± 4.83 Mpc)[1]
Apparent magnitude (V)13.5[1]
Characteristics
TypeSAc[1]
Size~129,400 ly (39.66 kpc) (estimated)[1]
Apparent size (V)1.2' x 0.7'[1]
Other designations
IRAS 04259-4216, 2MASX J04273300-4209549, MCG -07-10-006, PGC 15150, ESO 303- G 018[1]

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.[3]

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.[4]

See also

edit

References

edit
  1. ^ a b c d e f g h i j "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. 1585&rft.aulast=Seligman&rft.aufirst=Courtney&rft_id=https://cseligman.com/text/atlas/ngc15a.htm#1585&rfr_id=info:sid/en.wikipedia.org:NGC 1585" class="Z3988">
  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. 2023vio&rft_id=https://www.wis-tns.org/object/2023vio&rfr_id=info:sid/en.wikipedia.org:NGC 1585" class="Z3988">
edit