Two-dimensional resonance patterns in the discs of spiral galaxies
            
    Two major features of structure in galaxy discs: the long-term presence of spiral arms, and the continuous presence of OB stars concentrated in the arms, can be explained if a spiral density wave in the stellar population interacts with star-forming gas in the disc. With a recent method we are able to perform accurate characterization of the
            Beckman, J. et al.
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                        2020