The influence of streaming velocities and Lyman–Werner radiation on the formation of the first stars
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DOI: 10.1093/mnras/stab1953
Abstract: The first stars in the Universe, the so-called Population III stars, form in small dark matter minihaloes with virial temperatures Tvir < 104 K. Cooling in these minihaloes is dominated by molecular hydrogen (H2), and so… read more here.
Keywords: population iii; formation; first stars; lyman werner ... See more keywords