Simulated ELT/HARMONI observations of VCC 1861 show that a 2.5e5 solar mass IMBH (5% of the nuclear cluster mass) can be recovered from stellar kinematics at Virgo distance.
Currently, we knew that the stellar mass black holes (BHs, ๐๐ต๐ป โฒ 102๐โ) is massive star remnants [1]
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Extending the simulations of intermediate-mass black hole mass measurements to Virgo Cluster using ELT/HARMONI high resolution integral-field stellar kinematics
Simulated ELT/HARMONI observations of VCC 1861 show that a 2.5e5 solar mass IMBH (5% of the nuclear cluster mass) can be recovered from stellar kinematics at Virgo distance.