Radiative Transfer Modeling of an SN 1987A Light Echo—AT 2019xis

@article{Ding2021RadiativeTM,
  title={Radiative Transfer Modeling of an SN 1987A Light Echo—AT 2019xis},
  author={Jiachen Ding and Lifan Wang and Peter Brown and Ping Yang},
  journal={The Astrophysical Journal},
  year={2021},
  volume={919}
}
We use a Monte Carlo radiative transfer model (MCRTM) to simulate the UBVRI light curves, images, and linear polarization of a light echo from supernova SN 1987A in the Large Magellanic Cloud (LMC) using various dust cloud shapes, sizes, and optical properties. We compare the theoretical simulations to the observations of AT 2019xis, a light echo detected at a large angular distance (4.′05) from SN 1987A. We estimate the size and optical thickness of the dust cloud based on the simulation… 

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