NGC 633 explained

NGC 633
Constellation Name:Sculptor
Ra:01h 36m 23s
Dec:-37° 19’ 18”
Epoch:J2000
Appmag B:13.5
Sbrightness:22.37 mag/arcsec^2
Type:SBb

NGC 633 is a large barred spiral galaxy located in the constellation Sculptor. Its speed relative to the cosmic microwave background is 4,979 ± 18 km/s, which corresponds to a Hubble distance of 73.4 ± 5.2 Mpc (∼239 million ly).[1] NGC 633 was discovered by British astronomer John Herschel in 1834.

The luminosity class of NGC 633 is II and it has a broad HI line. It also contains regions of ionized hydrogen.

The smaller galaxy to the south of NGC 633 is PGC 5959 or ESO 297-012, and these two galaxies form a galactic pair.[2] The Hubble distance of ESO 297-012 is 73.51 ± 5.15,[3] which is almost identical to that of NGC 633, confirming that both galaxies are in gravitational interaction.[4] A contrast-enhanced image shows a bridge of matter between these two galaxies.

See also

External links

Notes and References

  1. Web site: By Name NASA/IPAC Extragalactic Database . 2024-07-23 . ned.ipac.caltech.edu.
  2. Web site: Soares . D.S.L. . de Souza . R.E. . de Carvalho . R.R. . Couto da Silva . T.C. . Southern Binary Galaxies I. A Sample of Isolated Pairs . July 22, 2024 . ArXiv.
  3. Web site: By Name NASA/IPAC Extragalactic Database . 2024-07-23 . ned.ipac.caltech.edu.
  4. Web site: New General Catalog Objects: NGC 600 - 649 . 2024-07-23 . cseligman.com.