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arXiv · astro-ph/9611118

Self-Microlensing in Compact Binary Systems

Bo Qin·Xiang-Ping Wu·Zhenlong Zou
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Abstract

The signature of the self-microlensing in compact binaries (white dwarfs, neutron stars and black holes) is a flare with the characteristic time of typically a few minutes. The probability of detecting these microlensing events can be as high as $1/50$ for a flux sensitivity of $Δm=0.01$ in magnitude. The discovery of the self-microlensing by binaries would furnish an additional way to find the masses of the lens and the companion and will be promising for the searches of black holes.

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Bo Qin, Xiang-Ping Wu, Zhenlong Zou. 1996-11-15. Self-Microlensing in Compact Binary Systems. https://doi.org/10.1088/0256-307x%2F14%2F2%2F022

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