We present a mechanism for β¦c β Ο + β¦(2012) production through an external emission Cabibbo favored weak decay mode, where the β¦( 2012) is dynamically generated from the interaction of KΞ * (1530), Ξ·β¦, with KΞ as the main decay channel. The β¦(2012) decays latter to KΞ in this picture, with results compatible with previous Belle data. The picture has as a consequence that one can evaluate the direct decay β¦ 0 c β Ο + K β Ξ 0 and the decay β¦ 0 c β Ο + KΞ * , Ο + Ξ·β¦ with direct coupling of KΞ * and Ξ·β¦ to K β Ξ 0 . We show that, within uncertainties and using data from a recent Belle measurement, all these three channels account for about (12-20)% of the total β¦c β Ο + K β Ξ 0 decay rate. The consistency of the molecular picture with all the data is established by showing that β¦c β Ξ 0 K * 0 β Ξ 0 K β Ο + together with β¦c β Ο + β¦ * β Ο + K β Ξ 0 account for about 85% of the total β¦c β Ο + K β Ξ 0 .