NGC 1134 explained

NGC 1134
Type:S
Dist Ly:35.16Mpc
Appmag V:13.05
Names: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.[1] 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.

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Notes and References

  1. Bizyaev DV, Zasov AV, Kaisin SS . 2001. Combined Color Indices and Photometric Structures of the Galaxies NGC 834 and NGC 1134. Astronomy Letters. 10.1134/1.1358378. 2001AstL...27..217B. 27. 4. 217–227. astro-ph/0001290 . 121528200.