NGC 2927 explained

NGC 2927
Constellation Name:Leo
Epoch:J2000
Type:SAB(rs)b[1]
Dist Ly:NaNMpc
Z:0.025147
H Radial V:7539 ± 2 km/s
Appmag V:12.9
Size V:1.3' x 1.0'
Size:~70.2kpc (estimated)

NGC 2927 is a 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).[2] The galaxy was discovered by German astronomer Heinrich d'Arrest on 21 February 1863.[3]

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.[4]

One supernova has been observed in NGC 2927: SN 2023uvg (type Ic, mag. 18.7).[5]

NGC 2927 forms a pair of galaxies with NGC 2929.[6]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 2927 . 14 August 2024.
  2. Web site: Distance Results for NGC 2927 . NASA/IPAC EXTRAGALACTIC DATABASE . NASA . 14 August 2024.
  3. Web site: NGC 2927 . Seligman . Courtney . Celestial Atlas . 14 August 2024 .
  4. Web site: SIMBAD astronomical database. NGC 2927 . . 14 August 2024.
  5. Web site: Transient Name Server . SN 2023uvg . . 14 August 2024.
  6. 10.1007/BF03036100 . Groups of galaxies. III. Some empirical characteristics . 1998 . Mahtessian . A. P. . Astrophysics . 41 . 3 . 308–321 . 1998Ap.....41..308M .