Draft:IC 5174
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| IC 5174 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Grus |
| Right ascension | 22h 12m 44.659s[1] |
| Declination | −38° 10′ 17.555″[1] |
| Redshift | 0.036832 ± 0.000470[2] |
| Apparent magnitude (B) | 14.63[2] |
| Characteristics | |
| Type | SB(s)b pec[1] |
| Size | ~689,000 ly (211.4 kpc) (estimated)[1] |
| Notable features | Seyfert 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 2 3 4 5 "NASA/IPAC Extragalactic Database (NED) results for object IC 5174". NASA/IPAC. Retrieved 2024-05-22.
- 1 2 3 "SIMBAD Astronomical Database - IC 5174". Centre de Données astronomiques de Strasbourg. Retrieved 2024-05-22.
- ↑ "Index Catalog Objects: IC 5150 - 5199". cseligman.com. Retrieved 2026-05-14.
- 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.
- ↑ 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.
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