Velocity Dispersions in Nucleus of M87 (repeat): Cycle 4 FOS Ero

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Hst Proposal Id #5634 Galaxies &Amp, Clusters

Scientific paper

The FOS will be used with a small aperture to map the stellar velocity
dispersion and rotation in the central region of NGC4486 = M87. The
velocity dispersions will be used to discriminate between the large M/Ls
required by massive black holes, velocity anisotropy, and isothermal
velocity distributions.

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