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NGC 4611

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Galaxy in the constellation Coma Berenices
NGC 4611
The intermediate spiral galaxy NGC 4611
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12 41 25.4331
Declination+13° 43′ 46.198″
Redshift0.020404
Heliocentric radial velocity6117 ± 1 km/s
Distance309.7 ± 21.7 Mly (94.94 ± 6.65 Mpc)
Apparent magnitude (V)14.3
Characteristics
TypeSbc C
Size~130,100 ly (39.89 kpc) (estimated)
Apparent size (V)1.2' x 0.2'
Other designations
IRAS F12389+1400, 2MASX J12412541+1343458, IC 805, UGC 7849, MCG +02-32-179, PGC 42564

NGC 4611 is a intermediate spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 6,437 ± 22 km/s, which corresponds to a Hubble distance of 94.9 ± 6.7 Mpc (∼310 million light-years). It was discovered by French astronomer Édouard Stephan on 17 May 1881. This galaxy was also observed by the American astronomer Lewis Swift on 20 April 1889, and listed in the Index Catalogue as IC 805.

According to the SIMBAD database, NGC 4611 is an Active Galaxy Nucleus Candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.

Supernova

One supernova has been observed in NGC 4611: SN 2023dtz (type Ia, mag. 18.1) was discovered by ATLAS on 21 March 2023.

See also

References

  1. ^ "Results for object NGC 4611". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 23 July 2024.
  2. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 4611". Celestial Atlas. Retrieved 13 December 2024.
  3. "NGC 4611". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 13 December 2024.
  4. "SN 2023dtz". Transient Name Server. IAU. Retrieved 13 December 2024.

External links

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New General Catalogue 4500 to 4999
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