Dwarf galaxies might not be the birth sites of supermassive black holes. (arXiv:1901.02895v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Mezcua_M/0/1/0/all/0/1">Mar Mezcua</a>
Intermediate-mass black holes (BHs) in local dwarf galaxies are considered
the relics of the early seed BHs. However, their growth might have been
impacted by galaxy mergers and BH feedback so that they cannot be treated as
tracers of the early seed BH population.
Intermediate-mass black holes (BHs) in local dwarf galaxies are considered
the relics of the early seed BHs. However, their growth might have been
impacted by galaxy mergers and BH feedback so that they cannot be treated as
tracers of the early seed BH population.
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