Microlensing of an extended source by a power-law mass distribution

@article{Congdon2007MicrolensingOA,
  title={Microlensing of an extended source by a power-law mass distribution},
  author={Arthur B. Congdon and C. Keeton and S. Osmer},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2007},
  volume={376},
  pages={263-272}
}
  • Arthur B. Congdon, C. Keeton, S. Osmer
  • Published 2007
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • Microlensing promises to be a powerful tool for studying distant galaxies and quasars. As the data and models improve, there are systematic effects that need to be explored. Quasar continuum and broad-line regions may respond differently to microlensing due to their different sizes; to understand this effect, we study microlensing of finite sources by a mass function of stars. We find that microlensing is insensitive to the slope of the mass function but does depend on the mass range. For… CONTINUE READING
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