NGC 1448

Galaxy in the constellation Horologium From Wikipedia, the free encyclopedia

NGC 1448 is an unbarred spiral galaxy seen nearly edge-on in the constellation Horologium. It is at a distance of 55 million light years from Earth. It was discovered by British astronomer John Herschel on 24 October 1835.[2] Herschel observed the galaxy again on 14 December 1835, resulting in it being listed twice in the New General Catalogue, as NGC 1448 and as NGC 1457.[2]

Right ascension03h 44m 31.8804s[1]
Declination−44° 38 41.15[1]
Redshift0.003896[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 1448
NGC 1448 by the Very Large Telescope
Observation data (J2000 epoch)
ConstellationHorologium
Right ascension03h 44m 31.8804s[1]
Declination−44° 38 41.15[1]
Redshift0.003896[1]
Heliocentric radial velocity1,168±2 km/s[1]
Distance56.5 ± 7.6 Mly (17.3 ± 2.3 Mpc)[1]
Apparent magnitude (V)10.7
Characteristics
TypeSAcd [1]
Size~142,800 ly (43.78 kpc) (estimated)[1]
Apparent size (V)7.6 × 1.7[1]
Other designations
ESO 249- G 016, IRAS 03428-4448, NGC 1457, MCG -07-08-005, PGC 13727[1]
Close

From the spectral analysis of SN 2001el, over a dozen diffuse interstellar bands were discovered in NGC 1448 – one of the few cases that these bands were observed outside of the Milky Way. However, the bands were significantly weaker at SN 2003hn.[3]

In January 2017 it was announced that evidence for a supermassive black hole in NGC 1448 had been found in the center of the galaxy.[4]

The galaxy belongs to the NGC 1433 group,[5] part of the Doradus cloud of galaxies.

Supernovae

Six supernovae have been observed in NGC 1448:

  • SN 1983S (Type II, mag. 14.5) was discovered by Robert Evans on 6 October 1983.[6][7]
  • SN 2001el (Type Ia, mag. 14.5) was discovered by Berto Monard on 17 September 2001.[8][9] It reached magnitude 12.3, making it the brightest supernova of 2001.[10]
  • SN 2003hn (Type II, mag. 14.1) was discovered by Robert Evans on 25 August 2003.[11][12]
  • SN 2014df (Type Ib, mag. 14) was discovered by Berto Monard on 3 June 2014.[13][14]
  • SN 2020zbv (Type IIP, mag. 18.83) was discovered by the Distance Less Than 40 Mpc Survey (DLT40) on 10 November 2020.[15]
  • SN 2021pit (Type Ia, mag. 13.5) was discovered by ASAS-SN on 10 June 2021.[16]

The galaxy in different wavelengths

See also

References

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