The origin of compact galaxies with anomalously high black hole masses
  Observations of local galaxies harbouring supermassive black holes (BHs) of
anomalously high mass, M_BH, relative to their stellar mass, M_star, appear to
be at odds with simple models of the co-evolution between galaxies and their
central BHs. We study the origin of such outliers in a Lambda cold dark matter
context using the EAGLE cosmological, hydrodynamical simulation. We find 15
'M_BH(M_star)-outlier' galaxies, defined as having M_BH more than 1.5 dex above
the median M_BH(M_star) relation in the simulation, M_{BH,med}. All
M_BH(M_star)-outliers are satellite galaxies, typically with M_star ~ 10^10
M_sun and M_BH ~ 10^8 M_sun. They have all become outliers due to a combination
of tidal stripping of their outer stellar component acting over several Gyr and
early formation times leading to rapid BH growth at high redshift, with the
former mechanism being most important for 67 per cent of these outliers. The
same mechanisms also cause the M_BH(M_star)-outlier satellites to be amongst
the most compact galaxies in the simulation, making them ideal candidates for
ultracompact dwarf galaxy progenitors. The 10 most extreme central galaxies
found at z=0 (with log_{10}(M_BH/M_{BH,med}) in [1.2, 1.5]) grow rapidly in
M_BH to lie well above the present-day M_BH-M_star relation at early times (z >
2), and either continue to evolve parallel to the z=0 relation or remain
unchanged until the present day, making them 'relics' of the high-redshift
universe. This high-z formation mechanism may help to explain the origin of
observed M_BH(M_star)-outliers with extended dark matter haloes and undisturbed
morphologies.
