NGC 1134
| NGC 1134 | |
|---|---|
 DSS picture of NGC 1134 | |
| Observation data (J2000 epoch) | |
| Constellation | Aries |
| Right ascension | 02h 53m 41.341s[1] |
| Declination | +13° 00′ 50.85″[1] |
| Redshift | 0.012178 ± 0.000010[2] |
| Distance | 114.7 Mly (35.16 Mpc)[3] |
| Apparent magnitude (V) | 13.05[4] |
| Characteristics | |
| Type | S[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 | |
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.
References
- ^ a b c Skrutskie, M. F.; et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.
- ^ 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.
- ^ 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, 86.
- ^ a b "NASA/IPAC Extragalactic Database", Results for NGC 1134, nasa, retrieved 2010-05-10.
- ^ 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.
External links
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