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NGC 2927

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Galaxy in the constellation Leo

NGC 2927
The barred spiral galaxy NGC 2927
Observation data (J2000 epoch)
ConstellationLeo
Right ascension09 37 15.21
Declination+23° 35′ 26.209″
Redshift0.025147
Heliocentric radial velocity7539 ± 2 km/s
Distance376.7 ± 26.4 Mly (115.49 ± 8.09 Mpc)
Apparent magnitude (V)12.9
Characteristics
TypeSAB(rs)b
Size~229,000 ly (70.20 kpc) (estimated)
Apparent size (V)1.3′ × 1.0′
Other designations
IRAS F09343+2349, 2MASX J09371521+2335261, UGC 5122, MCG +04-23-016, PGC 27385, CGCG 122-032

NGC 2927 is a large barred spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 7830 ± 20 km/s, which corresponds to a Hubble distance of 115.49 ± 8.09 Mpc (∼377 million light-years). In addition, three non-redshift measurements give a distance of 120.667 ± 0.882 (∼394 million light-years). The galaxy was discovered by German astronomer Heinrich d'Arrest on 21 February 1863.

The SIMBAD database lists NGC 2927 as a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure.

One supernova has been observed in NGC 2927: SN 2023uvg (type Ic, mag. 18.7389) was discovered by the Automatic Learning for the Rapid Classification of Events (ALeRCE) on 13 October 2023.

NGC 2927 forms a pair of galaxies with NGC 2929.

See also

References

  1. ^ "Results for object NGC 2927". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 14 August 2024.
  2. "Distance Results for NGC 2927". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 14 August 2024.
  3. Seligman, Courtney. "NGC 2927". Celestial Atlas. Retrieved 14 August 2024.
  4. "NGC 2927". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 December 2024.
  5. "SN 2023uvg". Transient Name Server. IAU. Retrieved 14 August 2024.
  6. Mahtessian, A. P. (1998). "Groups of galaxies. III. Some empirical characteristics". Astrophysics. 41 (3): 308–321. Bibcode:1998Ap.....41..308M. doi:10.1007/BF03036100.

External links

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