Modeling the Infrared Emission from the Eridani Disk

@article{Li2003ModelingTI,
  title={Modeling the Infrared Emission from the Eridani Disk},
  author={Aigen Li and Jonathan I. Lunine and George J Bendo},
  journal={The Astrophysical Journal},
  year={2003},
  volume={598}
}
We model the infrared (IR) emission from the ringlike dust disk around the main-sequence (MS) star Eridani, a young analog to our solar system, in terms of a porous dust model previously developed for the extended wedge-shaped disk around the MS star β Pictoris and the sharply truncated ringlike disks around the Herbig Ae/Be stars HR 4796A and HD 141569A. It is shown that the porous dust model with a porosity of ~90% is also successful in reproducing the IR to submillimeter dust emission… 

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