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The 30 Doradus Nebula in the Large Magellanic Cloud (LMC) contains themassive starburst cluster NGC 2070 with a massive and probably younger stellarsub clump at its center: R136. It is not clear how such a massive inner clustercould form several million years after the older stars in NGC 2070, given thatstellar feedback is usually thought to expel gas and inhibit further starformation. Using the recently developed 1D feedback scheme WARPFIELD to scan alarge range of cloud and cluster properties, we show that an age offset ofseveral million years between the stellar populations is in fact to be expectedgiven the interplay between feedback and gravity in a giant molecular cloud(GMC) with a density $\gtrsim 500$ cm$^{-3}$ due to re-accretion of gas ontothe older stellar population. Neither capture of field stars nor gas retentioninside the cluster have to be invoked in order to explain the observed ageoffset in NGC 2070 as well as the structure of the interstellar medium (ISM)around it.

Forming clusters within clusters: How 30 Doradus recollapsed and gave birth again