Examine the second link that I posted. "For these conditions, the detailed properties of the outflow determine whether a full r-process can or cannot occur, im

Examine the second link that I posted. "For these conditions, the detailed properties of the outflow determine whether a full r-process can or cannot occur, implying that a wide range of observable phenomena is possible. We show that on average the disk outflow lanthanide fraction is suppressed relative to the solar isotopic pattern. In combination with the dynamical ejecta, these outflows imply a kilonova with both blue and red components."