  The link between hot and cool stellar outflows is shown to be critical for
correctly predicting the masses of the most massive black holes (BHs) below the
so-called pair-instability supernova (PISN) mass gap. Gravitational Wave (GW)
event 190521 allegedly hosted an "impossibly" heavy BH of 85 Solar Masses. Here
we show how our increased knowledge of both metallicity Z and temperature
dependent mass loss is critical for our evolutionary scenario of a low-Z blue
supergiant (BSG) progenitor of an initially approx 100 Solar Masses star to
work. We show using MESA stellar evolution modelling experiments that as long
as we can keep such stars above 8000 K such low-Z BSGs can avoid strong winds,
and keep a very large envelope mass intact before core collapse. This naturally
leads to the Cosmic Time dependent maximum BH function below the PISN gap.
