A SCUBA survey of the NGC 2068/2071 protoclusters

We report the results of a submillimeter dust continuum survey of the protoclusters NGC 2068 and NGC 2071 in Orion B carried out at $850 \mu$m and $450 \mu$m with SCUBA on JCMT. The mapped region is ~$32\arcmin \times 18\arcmin$ in size (~4 pc $\times$ 2 pc) and consists of filamentary dense cores which break up into small-scale (~5 000 AU) fragments, including 70 starless condensations and 5 circumstellar envelopes/disks. The starless condensations, seen on the same spatial scales as protostellar envelopes, are likely to be gravitationally bound and pre-stellar in nature. Their mass spectrum, ranging from ~0.3 $M_\odot$ to ~5 $M_\odot$, is reminiscent of the stellar initial mass function (IMF). Their mass-size relation suggests that they originate from gravitationally-driven fragmentation. We thus argue that pre-collapse cloud fragmentation plays a major role in shaping the IMF