“School of Astronomy”
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| Paper IPM / Astronomy / 11551 |
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We report the result of the analysis of a dramatic repeating gravitational microlensing event OGLE-2009-BLG-
092/MOA-2009-BLG-137, for which the light curve is characterized by two distinct peaks with perturbations near
both peaks. We find that the event is produced by the passage of the source trajectory over the central perturbation
regions associated with the individual components of a wide-separation binary.
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