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NGC 1134 is a spiral galaxy in the Aries constellation. It has a highly inclined disk, with respect to the line of sight from Earth. There is a weak outer extension of the spiral structure in this galaxy. It has been listed in the Arp Atlas of Peculiar Galaxies (Arp number 200), under the "Galaxies with material ejected from nuclei" section.[5] NGC 1134 is classified as a galaxy with reduced surface brightness, and it possesses a distinct bulge in its centre, as judged by photometric analysis. It has a small and distant companion about 7' to the south.

NGC 1134
DSS picture of NGC 1134
Observation data (J2000 epoch)
ConstellationAries
Right ascension02h 53m 41.341s[1]
Declination+13° 00′ 50.85″[1]
Redshift0.012178 ± 0.000010[2]
Distance114.7 Mly (35.16 Mpc)[3]
Apparent magnitude (V)13.05[4]
Characteristics
TypeS[4]
Apparent size (V)1.467′ × 0.997′[1]
Other designations
2MASX J02534134+1300508, APG 200, ARP 200, BWE 0250+1248, IRAS 02509+1248, LEDA 10928, MCG+02-08-027, PGC 10928, UGC 2365, UZC J025341.2+130053, Z 0250.9+1248, Z 440-27, ZWG 440.27

References


  1. Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131: 1163–1183. doi:10.1086/498708. ISSN 0004-6256.
  2. Oosterloo, T.; Shostak, S. (June 1993), "H I observations of binary spiral galaxies", Astronomy and Astrophysics Supplement Series, 99 (2): 379–406, Bibcode:1993A&AS...99..379O.
  3. Tully, R. Brent; et al. (October 2013), "Cosmicflows-2: The Data", The Astronomical Journal, 146 (4): 25, arXiv:1307.7213, Bibcode:2013AJ....146...86T, doi:10.1088/0004-6256/146/4/86, S2CID 118494842, 86.
  4. "NASA/IPAC Extragalactic Database", Results for NGC 1134, nasa, retrieved 2010-05-10.
  5. Bizyaev DV, Zasov AV, Kaisin SS (2001). "Combined Color Indices and Photometric Structures of the Galaxies NGC 834 and NGC 1134". Astronomy Letters. 27 (4): 217–227. arXiv:astro-ph/0001290. Bibcode:2001AstL...27..217B. doi:10.1134/1.1358378. S2CID 121528200.



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[de] NGC 1134

NGC 1134 ist eine Spiralgalaxie vom Hubble-Typ Sb[2] mit ausgedehnten Sternentstehungsgebieten im Sternbild Widder am Nordsternhimmel. Sie ist schätzungsweise 164 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 120.000 Lichtjahren. Gemeinsam mit IC 267 bildet sie ein wahrscheinlich gravitativ gebundenes Galaxienpaar. Im selben Himmelsareal befinden sich u. a. die Galaxien NGC 1115, NGC 1116, NGC 1117, NGC 1127.
- [en] NGC 1134

[ru] NGC 1134

NGC 1134 (другие обозначения — UGC 2365, MCG 2-8-27, ZWG 440.27, ARP 200, IRAS02509+1248, PGC 10928) — спиральная галактика (Sb) в созвездии Овен.


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