The very careful Event Horizon Telescope estimate of the mass of the
supermassive black hole at the center of the Giant CD galaxy M87, allied with
recent high quality photometric and spectroscopic measurements, yields a proper
dark/luminous mass decomposition from the galaxy center to its virial radius.
That provides us with decisive information on crucial cosmological and
astrophysical issues. The dark and the standard matter distributions in a wide
first time detected galaxy region under the supermassive black hole
gravitational control. The well known supermassive black hole mass vs stellar
dispersion velocity relationship at the highest galaxy masses implies an exotic
growth of the former. This may be the first case in which one can argue that
the supermassive black hole mass growth was also contributed by the Dark Matter
component. A huge dark matter halo core in a galaxy with inefficient baryonic
feedback is present and consequently constrains the nature of the dark halo
particles. The unexplained entanglement between dark/luminous structural
properties, already emerged in disk systems, also appears.
LEG[A]CY | 14 August 2016 by Protobacillus
















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