A consistent microlensing model for the Galactic bar

@article{Zhao1996ACM,
  title={A consistent microlensing model for the Galactic bar},
  author={HongSheng Zhao and Robert Michael Rich and David N. Spergel},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={1996},
  volume={282},
  pages={175-181}
}
We compute a microlensing map for the Galactic bar. The predicted event rate and event duration distribution are consistent with the 55 events recently reported by the MACHO and OGLE collaborations. Most of the events are due to lensing by stars in the near end of the bar_ Lens mass functions with about 30-60 per cent of the lens mass as brown dwarfs are rejected at 20'-60' levels_ To make our model useful for other workers, we tabulate the optical depth of the bar and average event duration… 

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References

preprint MACHO-Bulge-002; \Microlensing Workshop