Other
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5267h&link_type=abstract
HST Proposal ID #5267
Other
Hst Proposal Id #5267 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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