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.
Fecha de publicación:
7
2020