NGC 2648 explained

NGC 2648
Constellation Name:Cancer
Sbrightness:23.61 mag/arcsec²
Epoch:J2000
Type:SAa
Names:PGC 24464, ARP 89, UGC 4541, MCG 2-22-5, CGCG 60-35, KCPG 168A
Appmag B:12.8
Appmag V:11.82

NGC 2648 is a spiral galaxy located in the constellation Cancer. Its speed relative to the cosmic microwave background is 2,451 ± 19 km/s, which corresponds to a Hubble distance of 36.2 ± 2.6 Mpc (∼118 million ly).[1] NGC 2648 was discovered by German-British astronomer William Herschel in 1784.

The galaxies PGC 24469 and NGC 2648 are designated in Halton Arp's Atlas of Peculiar Galaxies as Arp 89.[2]

The luminosity class of NGC 2648 is I and it has a broad HI line.

NGC 2648 is a retired galaxy, which is a galaxy in which star formation has practically ceased is said to be passive. However, some passive galaxies may still show faint emission lines similar to those of LINER galaxies. This is what a team of French and Brazilian astronomers discovered. It is from them that the name retired galaxy comes.[3]

To date, three non-redshift measurements give a distance of 34.333 ± 0.231 Mpc (∼112 million ly), which is within the Hubble distance values.[4]

See also

External links

References

  1. Web site: By Name NASA/IPAC Extragalactic Database . 2024-07-03 . ned.ipac.caltech.edu.
  2. Web site: New General Catalog Objects: NGC 2600 - 2649 . 2024-07-03 . cseligman.com.
  3. Web site: titre : Retired galaxies behaving like active galaxies . 2024-07-03 . Observatoire de Paris - PSL - Centre de recherche en astronomie et astrophysique . en.
  4. Web site: NED Query Results for NGC 2648 . 2024-07-03 . ned.ipac.caltech.edu.