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A ring-like filament of stars wrapping around the Milky Way may actually belong to the galaxy itself, rippling above and below the relatively flat galactic plane. If so, that would expand the size of the known galaxy by 50% and raise intriguing questions about what caused the waves of stars.
Scientists used data collected by the Sloan Digital Sky Survey to reanalyze the brightness and distance of stars at the edge of the galaxy. They found that the fringe of the disk is puckered into ridges and grooves of stars, like corrugated cardboard.
"It looks to me like maybe these patterns are following the spiral structure of the Milky Way, so they may be related," astronomer Heidi Newberg, with Rensselaer Polytechnic Institute in New York, told Discovery News. Read more...
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