An isolated mass gap black hole or neutron star detected with astrometric microlensing

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An isolated mass gap black hole or neutron star detected with astrometric microlensing
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Astronomers may have detected a 'dark' free-floating black hole AAS_Office AAS_Publishing

We present the analysis of five black hole candidates identified from gravitational microlensing surveys. Hubble Space Telescope astrometric data and densely sampled lightcurves from ground-based microlensing surveys are fit with a single-source, single-lens microlensing model in order to measure the mass and luminosity of each lens and determine if it is a black hole.

This compact object lens is relatively nearby and has a slow transverse motion of $<$30 km/s. OB110462 shows significant tension between models well-fit to photometry vs. astrometry, making it currently difficult to distinguish between a neutron star and a black hole. Additional observations and modeling with more complex system geometries, such as binary sources are needed to resolve the puzzling nature of this object.

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