Two growing modes and the morphology–quiescence relation in isolated galaxies

@article{Woo2019TwoGM,
  title={Two growing modes and the morphology–quiescence relation in isolated galaxies},
  author={Joanna Woo and Sara L. Ellison},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2019}
}
  • J. Woo, S. Ellison
  • Published 29 October 2018
  • Physics
  • Monthly Notices of the Royal Astronomical Society
Quiescence in galaxies correlates strongly with the central density/morphology of the stellar distribution. We investigate two possible explanations for this morphology-quiescence relation: 1) the central density results from a dissipative core-building event (`compaction') that feeds an AGN that quenches the galaxy and 2) the central density results from inside-out growth by galaxy-wide star formation that is quenched by processes unrelated to the central density. We aim to distinguish these… Expand

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