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What happens when you take observations of a gas cloud, a protostar, and a pre-star dense core of gas, and model them with turbulence A downright hypnotizing model at how multiple star systems may form. A gas cloud 450 light years away in the constellation Taurus hosts not just a newborn
stanley cup protostar, but a dense core of gas that will likely become a star in the near future. Observations of this system have led to new simulations on the role of turbulence in the formation of multiple star systems. We know the conditions necessary to form stars: clouds with a few solar masses worth of gas and dust contained within a tenth of a light-year, enough time for things to clomp together, and sooner or later fusion will start. What we aren ;t so sure about is the distribution and kinematics of that gas and dust lead
stanley cup ing up to core formation and the birth of a protostar. The only way to pin those conditions down are to observe brand-new protostars, and hopefully find a few almost-star gas cores before they kick off fusion. Protostars only last
stanley thermos mug a few hundred thousand years swaddled in gas and dust before they either incorporate the material or blow it away, entering the next stage of its multi-billion year lifetime. Multi-wavelength composite of MC27: low-density green, ALMA and high-density emission red, ALMA of the dust and gas cloud, and the protostar infrared emission blue, Spitzer . Credit: Kazuki Tokuda Osaka Prefecture University / ALMA ESO/NAOJ/NRAO / NASA