THE FORMATION OF MASSIVE POPULATION III STARS IN THE PRESENCE OF TURBULENCE
THE FORMATION OF MASSIVE POPULATION III STARS IN THE PRESENCE OF TURBULENCE
Population III stars forming in the infant universe at z=30 heralded the end of the cosmic dark ages. They are presumed to be assembled in so-called minihaloes with virial temperatures of a few thousand K where collapse is triggered by molecular hydrogen cooling. A central question concerns their final masses, …