Edge Rewrite
// request.cf · coarse context

A page that knows where it met you.

Only coarse request metadata is shown. This demo does not display or persist visitor IP addresses.

Country
US
Cloudflare location
CMH
Connection
HTTP/2
Language
Not provided

Ray ID: a44b1b7b88324afc

Jump to content

Draft:IC 5174

From Wikipedia, the free encyclopedia
IC 5174
Above is IC 5175 Below is IC 5174
Observation data (J2000 epoch)
ConstellationGrus
Right ascension22h 12m 44.659s[1]
Declination−38° 10′ 17.555″[1]
Redshift0.036832 ± 0.000470[2]
Apparent magnitude (B)14.63[2]
Characteristics
TypeSB(s)b pec[1]
Size~689,000 ly (211.4 kpc) (estimated)[1]
Notable featuresSeyfert galaxy[2]
Other designations
ESO 344-013, ESO 220947-3825.2, AM 2209-382 NED01, MCG -06-48-028, PGC 68292[1]

IC 5174 is a barred spiral galaxy in constellation Grus. It was discovered in year 1899, by DeLisle Stewart.[3] The interacting galaxy pair IC 5174/75 has drawn attention, due to an angular size for IC 5174 that is disproportionate to its brightness.[4] A preliminary investigation of this peculiar system is given, based on two ESO Schmidt plates and digital spectra of the two galaxies.[4]

The two long outer arms of IC 5174 measure approximately 300 kpc[4]. IC 5174 was involved in a 1998 study measuring neutral hydrogen lines in galaxies.[5]

See Also

[edit]

References

[edit]
  1. 1 2 3 4 5 "NASA/IPAC Extragalactic Database (NED) results for object IC 5174". NASA/IPAC. Retrieved 2024-05-22.
  2. 1 2 3 "SIMBAD Astronomical Database - IC 5174". Centre de Données astronomiques de Strasbourg. Retrieved 2024-05-22.
  3. ↑ "Index Catalog Objects: IC 5150 - 5199". cseligman.com. Retrieved 2026-05-14.
  4. 1 2 3 West, R. M.; Barbier, R. (February 1982). "The very large, interacting galaxy pair IC 5174/75". Astronomy and Astrophysics. 106: 53–57. Bibcode:1982A&A...106...53W.
  5. ↑ Theureau, G.; Bottinelli, L.; Coudreau-Durand, N.; Gouguenheim, L.; Hallet, N.; Loulergue, M.; Paturel, G.; Teerikorpi, P. (June 1998). "Kinematics of the local universe". Astronomy and Astrophysics Supplement. 130: 333–339.