Langbahn Team – Weltmeisterschaft

NGC 4611

NGC 4611
The intermediate spiral galaxy NGC 4611
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 41m 25.4331s[1]
Declination+13° 43′ 46.198″[1]
Redshift0.020404[1]
Heliocentric radial velocity6117 ± 1 km/s[1]
Distance309.7 ± 21.7 Mly (94.94 ± 6.65 Mpc)[1]
Apparent magnitude (V)14.3[1]
Characteristics
TypeSbc C[1]
Size~130,100 ly (39.89 kpc) (estimated)[1]
Apparent size (V)1.2' x 0.2'[1]
Other designations
IRAS F12389+1400, 2MASX J12412541+1343458, IC 805, UGC 7849, MCG +02-32-179, PGC 42564[1]

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).[1] It was discovered by French astronomer Édouard Stephan on 17 May 1881.[2] This galaxy was also observed by the American astronomer Lewis Swift on 20 April 1889, and listed in the Index Catalogue as IC 805.[2]

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.[3]

Supernova

One supernova has been observed in NGC 4611: SN 2023dtz (type Ia, mag. 18.1) was discovered by ATLAS on 21 March 2023.[4]

See also

References

  1. ^ a b c d e f g h i j k "Results for object NGC 4611". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 23 July 2024.
  2. ^ a b 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.