Ionization: a possible explanation for the difference of mean disk sizes in star-forming regions

@article{Kuffmeier2020IonizationAP,
  title={Ionization: a possible explanation for the difference of mean disk sizes in star-forming regions},
  author={M. Kuffmeier and B. Zhao and Paola Caselli},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2020}
}
Surveys of protoplanetary disks in star-forming regions of similar age revealed significant variations in average disk mass between some regions. For instance, disks in the Orion Nebular Cluster (ONC) and Corona Australis (CrA) are on average smaller than disks observed in Lupus, Taurus, Chamaeleon I or Ophiuchus. In contrast to previous models that study truncation of disks at a late stage of their evolution, we investigate whether disks may already be born with systematically smaller disk… Expand

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