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Astrometric Microlensing of Distant Sources due to the Stars in the Galaxy

Mareki Honma·Tomoharu Kurayama
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Abstract

We investigate properties of astrometric microlensing of distant sources (such as QSOs and radio galaxies) caused by stars in the Galaxy, mainly focusing on application to the VERA (VLBI Exploration of Radio Astrometry) project. Assuming typical parameters for the Galaxy disk and bulge, we show that the maximum optical depth for astrometric shift of 10 micro-arcsec level is 8.9x10^{-2} for QSO-disk lensing case and 3.8x10^{-2} for QSO-bulge lensing case. We also find that the maximum optical depth for QSO-disk lensing is larger by an order of magnitude than that for disk-disk or bulge-disk lensing case (assuming a typical source distance of 8 to 10 kpc). In addition to optical depth, we also calculate the event rate and find that the maximum event rate for QSO-disk lensing case is 1.2x10^{-2} event per year, which is about 30 times greater than that for disk-disk lensing case. This high event rate implies that if one monitors 10 QSOs behind the Galactic center region for 10 years, at least one astrometric microlensing event should be detected. Therefore, monitoring distant radio sources with VERA can be a new tool to study astrometric microlensing caused by stars in the Galaxy. We discuss the implications of astrometric microlensing for VERA by focusing on estimating the lens mass, and also present some possible candidates of radio sources toward which astrometric microlensing events should be searched for with VERA. (abridged)

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Mareki Honma, Tomoharu Kurayama. 2002-01-04. Astrometric Microlensing of Distant Sources due to the Stars in the Galaxy. https://doi.org/10.1086/339160

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