Morphology of Spitzer 24 μm Detected Galaxies in the UDF: The Links between Star Formation and Galaxy Morphology

@article{Shi2006MorphologyOS,
  title={Morphology of Spitzer 24 $\mu$m Detected Galaxies in the UDF: The Links between Star Formation and Galaxy Morphology},
  author={Y. Shi and George H. Rieke and Casey Papovich and Pablo G. P{\'e}rez-Gonz{\'a}lez and Emeric Le Floch},
  journal={The Astrophysical Journal},
  year={2006},
  volume={645},
  pages={199-208}
}
We have studied the morphologies of infrared-luminous galaxies at 0.3 ≤ z 1011 L☉]. We find that the high-redshift samples are dominated by galaxies with concentrations similar to local late-type disk galaxies; however, they are significantly more asymmetric than most local galaxies but are similar in both regards to local LIRGs. On average, the high-redshift infrared-active galaxies are slightly more asymmetric than the less active ones, although they do include a significantly higher portion… 

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