NGC 247

Source: Wikipedia, the free encyclopedia.
UGCA 11, PGC 2758,[1] Caldwell
62
Center of NGC 247 taken by Hubble Space Telescope.[2]

NGC 247 (also known as Caldwell 62 and commonly known as the Claw Galaxy

12.2 Mly away, but this was proved to be wrong.[4] NGC 247 is a member of the Sculptor Group, and is 70 000 light years in diameter. [5]

NGC 247 has an unusually large void on one side of its spiral disk. This void contains some older, redder stars but no younger, bluer stars.[6]

Nearby galaxies and galaxy group information

NGC 247 is one of several galaxies that is gravitationally bound to the Sculptor Galaxy (NGC 253). These galaxies form a small core in the center of the Sculptor Group, which is one of the nearest groups of galaxies to the Milky Way.[7] Most other galaxies associated with the Sculptor Group are only weakly gravitationally bound to this core.[7][8]

References

  1. ^ a b c d e f "NASA/IPAC Extragalactic Database". Results for NGC 247. Retrieved 2006-12-19.
  2. ^ "The centre of NGC 247". www.spacetelescope.org. Retrieved 6 October 2016.
  3. .
  4. ^ ""eso1107 — Photo Release: The Dusty Disc of NGC 247"". www.eso.org. Retrieved 24 Jul 2022.[1]
  5. ^ "NGC 247, an intermediate spiral galaxy in Cetus". Anne's Astronomy News (in Dutch). 2013-12-05. Retrieved 2020-04-16.
  6. ^ Wagner-Kaiser, R.; Demaio, T.; Sarajedini, A.; Chakrabarti, S. (2014). "The Void in the Sculptor Group Spiral Galaxy NGC 247". Monthly Notices of the Royal Astronomical Society. 443 (4): 3260–3269. .
  7. ^ a b Karachentsev, I. D. (2005). "The Local Group and Other Neighboring Galaxy Groups".
    S2CID 119385141
    .
  8. ^ Karachentsev, I. D.; Grebel, E. K.; Sharina, M. E.; Dolphin, A. E.; Geisler, D.; Guhathakrta, P.; Hodge, P. W.; Karachentseva, V. E.; Sarajedini, A.; Seitzer, P. (2003). "Distances to nearby galaxies in Sculptor".
    S2CID 54977869
    .

External links