The Leo ring is a massive, 200-kpc-wide structure orbiting the galaxies M105 and NGC3384 with a 4-Gyr period. This paper reports ultraviolet light originating from gaseous substructures, which is attributed to recent massive star formation. If structures like the Leo ring were common in the early Universe, they may have produced a large, yet undetected population of faint, metal-poor, halo-lacking dwarf galaxies.
- David A. Thilker
- Jennifer Donovan
- Mark Seibert