Kathryn's wheel: A spectacular galaxy collision discovered in the Galactic neighbourhood

Quentin A. Parker, Albert A. Zijlstra, Milorad Stupar, Michelle Cluver, David J. Frew, George Bendo, Ivan Bojičić

Research output: Contribution to journalArticlepeer-review

5 Citations (Scopus)


We report the discovery of the closest collisional ring galaxy to the Milky Way. Such rare systems occur due to 'bulls-eye' encounters between two reasonably matched galaxies. The recessional velocity of about 840 km s-1 is low enough that it was detected in the Anglo-AustralianObservatory/UK Schmidt Telescope Survey forGalactic H α emission. The distance is only-10 Mpc and the main galaxy shows a full ring of star-forming knots, 6.1 kpc in diameter surrounding a quiescent disc. The smaller assumed 'bullet' galaxy also shows vigorous star formation. The spectacular nature of the object had been overlooked because of its location in the Galactic plane and proximity to a bright star and even though it is the 60th brightest galaxy in the HI Parkes All Sky Survey (HIPASS) HI survey. The overall system has a physical size of-15 kpc, a total mass of M* = 6.6 × 109 M (stars + HI), a metallicity of [O/H]--0.4, and a star formation rate of 0.2-0.5 M yr-1, making it a Magellanictype system. Collisional ring galaxies therefore extend to much lower galaxy masses than commonly assumed. We derive a space density for such systems of 7 × 10-5 Mpc-3, an order of magnitude higher than previously estimated. This space density suggests Kathryn's Wheel is the nearest such system. We present discovery images, CTIO 4-m telescope narrow-band follow-up images and spectroscopy for selected emission components. Given its proximity and modest extinction along the line of sight, this spectacular system provides an ideal target for future high spatial resolution studies of such systems and for direct detection of its stellar populations.

Original languageEnglish
Pages (from-to)3759-3775
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Issue number4
Publication statusPublished - 1 Oct 2015
Externally publishedYes


  • Galaxies: groups: general
  • Galaxies: individual (ESO 179-13)
  • Galaxies: interactions
  • Galaxies: kinematics and dynamics
  • Galaxies: star formation


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