Astrometric microlensing: a channel to detect multiple lens systems

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Due to dramatic improvements in the precision of astrometric measurements, the observation of light centroid shifts in observed stars due to intervening massive compact objects (‘astrometric microlensing’) will become possible in the near future. Upcoming space missions, such as SIM and GAIA, will provide measurements with an accuracy of 4–60 μas depending on the magnitude of the observed stars...

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2002

ISSN: 0035-8711,1365-2966

DOI: 10.1046/j.1365-8711.2002.05608.x